Serveur d'exploration sur Caltech

Attention, ce site est en cours de développement !
Attention, site généré par des moyens informatiques à partir de corpus bruts.
Les informations ne sont donc pas validées.

Infrared emission from the solar neighborhood

Identifieur interne : 000327 ( Main/Corpus ); précédent : 000326; suivant : 000328

Infrared emission from the solar neighborhood

Auteurs : F. Boulanger ; M. Pérault

Source :

RBID : ISTEX:3CF0C26C5FE45C42C57581429DB0F9C1537ED48A

Abstract

Abstract: The main results of an extensive study of the infrared emission from the nearby interstellar medium are presented. These results are used to discuss the origin of the infrared emission from the solar neigbourhood. We show that altough most of the emission comes from interstellar matter not associated with current star formation, about half of the heating of grains is provided by ultraviolet photons radiated by stars younger than few 108 yrs.

Url:
DOI: 10.1007/BFb0118797

Links to Exploration step

ISTEX:3CF0C26C5FE45C42C57581429DB0F9C1537ED48A

Le document en format XML

<record>
<TEI wicri:istexFullTextTei="biblStruct">
<teiHeader>
<fileDesc>
<titleStmt>
<title xml:lang="en">Infrared emission from the solar neighborhood</title>
<author>
<name sortKey="Boulanger, F" sort="Boulanger, F" uniqKey="Boulanger F" first="F." last="Boulanger">F. Boulanger</name>
<affiliation>
<mods:affiliation>IPAC, Caltech, 100-22, 91125, Pasadena, CA, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Perault, M" sort="Perault, M" uniqKey="Perault M" first="M." last="Pérault">M. Pérault</name>
<affiliation>
<mods:affiliation>Ecole Normale Supérieure, 24 rue Lhomond, 75016, Paris, France</mods:affiliation>
</affiliation>
</author>
</titleStmt>
<publicationStmt>
<idno type="wicri:source">ISTEX</idno>
<idno type="RBID">ISTEX:3CF0C26C5FE45C42C57581429DB0F9C1537ED48A</idno>
<date when="1988" year="1988">1988</date>
<idno type="doi">10.1007/BFb0118797</idno>
<idno type="url">https://api.istex.fr/document/3CF0C26C5FE45C42C57581429DB0F9C1537ED48A/fulltext/pdf</idno>
<idno type="wicri:Area/Main/Corpus">000327</idno>
</publicationStmt>
<sourceDesc>
<biblStruct>
<analytic>
<title level="a" type="main" xml:lang="en">Infrared emission from the solar neighborhood</title>
<author>
<name sortKey="Boulanger, F" sort="Boulanger, F" uniqKey="Boulanger F" first="F." last="Boulanger">F. Boulanger</name>
<affiliation>
<mods:affiliation>IPAC, Caltech, 100-22, 91125, Pasadena, CA, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Perault, M" sort="Perault, M" uniqKey="Perault M" first="M." last="Pérault">M. Pérault</name>
<affiliation>
<mods:affiliation>Ecole Normale Supérieure, 24 rue Lhomond, 75016, Paris, France</mods:affiliation>
</affiliation>
</author>
</analytic>
<monogr></monogr>
<series>
<title level="s">Lecture Notes in Physics</title>
<imprint>
<date>1988</date>
</imprint>
<idno type="ISSN">0075-8450</idno>
<idno type="eISSN">1616-6361</idno>
<idno type="ISSN">0075-8450</idno>
</series>
<idno type="istex">3CF0C26C5FE45C42C57581429DB0F9C1537ED48A</idno>
<idno type="DOI">10.1007/BFb0118797</idno>
<idno type="ChapterID">16</idno>
<idno type="ChapterID">Chap16</idno>
</biblStruct>
</sourceDesc>
<seriesStmt>
<idno type="ISSN">0075-8450</idno>
</seriesStmt>
</fileDesc>
<profileDesc>
<textClass></textClass>
<langUsage>
<language ident="en">en</language>
</langUsage>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">Abstract: The main results of an extensive study of the infrared emission from the nearby interstellar medium are presented. These results are used to discuss the origin of the infrared emission from the solar neigbourhood. We show that altough most of the emission comes from interstellar matter not associated with current star formation, about half of the heating of grains is provided by ultraviolet photons radiated by stars younger than few 108 yrs.</div>
</front>
</TEI>
<istex>
<corpusName>springer</corpusName>
<author>
<json:item>
<name>F. Boulanger</name>
<affiliations>
<json:string>IPAC, Caltech, 100-22, 91125, Pasadena, CA, USA</json:string>
</affiliations>
</json:item>
<json:item>
<name>M. Pérault</name>
<affiliations>
<json:string>Ecole Normale Supérieure, 24 rue Lhomond, 75016, Paris, France</json:string>
</affiliations>
</json:item>
</author>
<language>
<json:string>eng</json:string>
</language>
<originalGenre>
<json:string>ReviewPaper</json:string>
</originalGenre>
<abstract>Abstract: The main results of an extensive study of the infrared emission from the nearby interstellar medium are presented. These results are used to discuss the origin of the infrared emission from the solar neigbourhood. We show that altough most of the emission comes from interstellar matter not associated with current star formation, about half of the heating of grains is provided by ultraviolet photons radiated by stars younger than few 108 yrs.</abstract>
<qualityIndicators>
<score>3.213</score>
<pdfVersion>1.3</pdfVersion>
<pdfPageSize>562 x 810 pts</pdfPageSize>
<refBibsNative>false</refBibsNative>
<keywordCount>0</keywordCount>
<abstractCharCount>455</abstractCharCount>
<pdfWordCount>2337</pdfWordCount>
<pdfCharCount>12501</pdfCharCount>
<pdfPageCount>8</pdfPageCount>
<abstractWordCount>73</abstractWordCount>
</qualityIndicators>
<title>Infrared emission from the solar neighborhood</title>
<chapterId>
<json:string>16</json:string>
<json:string>Chap16</json:string>
</chapterId>
<genre>
<json:string>conference</json:string>
</genre>
<serie>
<editor>
<json:item>
<name>H. Araki</name>
</json:item>
<json:item>
<name>J. Ehlers</name>
</json:item>
<json:item>
<name>K. Hepp</name>
</json:item>
<json:item>
<name>R. Kippenhahn</name>
</json:item>
<json:item>
<name>H. A. Weidenmüller</name>
</json:item>
<json:item>
<name>J. Wess</name>
</json:item>
<json:item>
<name>J. Zittartz</name>
</json:item>
</editor>
<issn>
<json:string>0075-8450</json:string>
</issn>
<language>
<json:string>unknown</json:string>
</language>
<eissn>
<json:string>1616-6361</json:string>
</eissn>
<title>Lecture Notes in Physics</title>
<copyrightDate>1988</copyrightDate>
</serie>
<host>
<editor>
<json:item>
<name>Andrew Lawrence</name>
</json:item>
</editor>
<subject>
<json:item>
<value>Physics and Astronomy</value>
</json:item>
<json:item>
<value>Physics</value>
</json:item>
<json:item>
<value>Astronomy</value>
</json:item>
<json:item>
<value>Astrophysics</value>
</json:item>
<json:item>
<value>Geophysics/Geodesy</value>
</json:item>
</subject>
<isbn>
<json:string>978-3-540-19052-3</json:string>
</isbn>
<language>
<json:string>unknown</json:string>
</language>
<eissn>
<json:string>1616-6361</json:string>
</eissn>
<title>Comets to Cosmology</title>
<bookId>
<json:string>3-540-19052-X</json:string>
</bookId>
<volume>297</volume>
<pages>
<last>129</last>
<first>122</first>
</pages>
<issn>
<json:string>0075-8450</json:string>
</issn>
<genre>
<json:string>book-series</json:string>
</genre>
<eisbn>
<json:string>978-3-540-39067-1</json:string>
</eisbn>
<copyrightDate>1988</copyrightDate>
<doi>
<json:string>10.1007/BFb0118781</json:string>
</doi>
</host>
<publicationDate>2008</publicationDate>
<copyrightDate>1988</copyrightDate>
<doi>
<json:string>10.1007/BFb0118797</json:string>
</doi>
<id>3CF0C26C5FE45C42C57581429DB0F9C1537ED48A</id>
<score>2.3424234</score>
<fulltext>
<json:item>
<original>true</original>
<mimetype>application/pdf</mimetype>
<extension>pdf</extension>
<uri>https://api.istex.fr/document/3CF0C26C5FE45C42C57581429DB0F9C1537ED48A/fulltext/pdf</uri>
</json:item>
<json:item>
<original>false</original>
<mimetype>application/zip</mimetype>
<extension>zip</extension>
<uri>https://api.istex.fr/document/3CF0C26C5FE45C42C57581429DB0F9C1537ED48A/fulltext/zip</uri>
</json:item>
<istex:fulltextTEI uri="https://api.istex.fr/document/3CF0C26C5FE45C42C57581429DB0F9C1537ED48A/fulltext/tei">
<teiHeader>
<fileDesc>
<titleStmt>
<title level="a" type="main" xml:lang="en">Infrared emission from the solar neighborhood</title>
<respStmt>
<resp>Références bibliographiques récupérées via GROBID</resp>
<name resp="ISTEX-API">ISTEX-API (INIST-CNRS)</name>
</respStmt>
</titleStmt>
<publicationStmt>
<authority>ISTEX</authority>
<publisher>Springer Berlin Heidelberg</publisher>
<pubPlace>Berlin, Heidelberg</pubPlace>
<availability>
<p>Springer-Verlag, 1988</p>
</availability>
<date>1988</date>
</publicationStmt>
<sourceDesc>
<biblStruct type="inbook">
<analytic>
<title level="a" type="main" xml:lang="en">Infrared emission from the solar neighborhood</title>
<author xml:id="author-1">
<persName>
<forename type="first">F.</forename>
<surname>Boulanger</surname>
</persName>
<affiliation>IPAC, Caltech, 100-22, 91125, Pasadena, CA, USA</affiliation>
</author>
<author xml:id="author-2">
<persName>
<forename type="first">M.</forename>
<surname>Pérault</surname>
</persName>
<affiliation>Ecole Normale Supérieure, 24 rue Lhomond, 75016, Paris, France</affiliation>
</author>
</analytic>
<monogr>
<title level="m">Comets to Cosmology</title>
<title level="m" type="sub">Proceedings of the Third IRAS Conference Held at Queen Mary College, University of London July 6–10, 1987</title>
<idno type="pISBN">978-3-540-19052-3</idno>
<idno type="eISBN">978-3-540-39067-1</idno>
<idno type="pISSN">0075-8450</idno>
<idno type="eISSN">1616-6361</idno>
<idno type="DOI">10.1007/BFb0118781</idno>
<idno type="book-ID">3-540-19052-X</idno>
<idno type="book-title-ID">22254</idno>
<idno type="book-sequence-number">297</idno>
<idno type="book-volume-number">297</idno>
<idno type="book-chapter-count">51</idno>
<editor>
<persName>
<forename type="first">Andrew</forename>
<surname>Lawrence</surname>
</persName>
</editor>
<imprint>
<publisher>Springer Berlin Heidelberg</publisher>
<pubPlace>Berlin, Heidelberg</pubPlace>
<date type="published" when="2008-01-29"></date>
<biblScope unit="volume">297</biblScope>
<biblScope unit="page" from="122">122</biblScope>
<biblScope unit="page" to="129">129</biblScope>
</imprint>
</monogr>
<series>
<title level="s">Lecture Notes in Physics</title>
<editor>
<persName>
<forename type="first">H.</forename>
<surname>Araki</surname>
</persName>
</editor>
<editor>
<persName>
<forename type="first">J.</forename>
<surname>Ehlers</surname>
</persName>
</editor>
<editor>
<persName>
<forename type="first">K.</forename>
<surname>Hepp</surname>
</persName>
</editor>
<editor>
<persName>
<forename type="first">R.</forename>
<surname>Kippenhahn</surname>
</persName>
</editor>
<editor>
<persName>
<forename type="first">H.</forename>
<forename type="first">A.</forename>
<surname>Weidenmüller</surname>
</persName>
</editor>
<editor>
<persName>
<forename type="first">J.</forename>
<surname>Wess</surname>
</persName>
</editor>
<editor>
<persName>
<forename type="first">J.</forename>
<surname>Zittartz</surname>
</persName>
</editor>
<biblScope>
<date>1988</date>
</biblScope>
<idno type="pISSN">0075-8450</idno>
<idno type="eISSN">1616-6361</idno>
<idno type="series-Id">5304</idno>
</series>
<idno type="istex">3CF0C26C5FE45C42C57581429DB0F9C1537ED48A</idno>
<idno type="DOI">10.1007/BFb0118797</idno>
<idno type="ChapterID">16</idno>
<idno type="ChapterID">Chap16</idno>
</biblStruct>
</sourceDesc>
</fileDesc>
<profileDesc>
<creation>
<date>1988</date>
</creation>
<langUsage>
<language ident="en">en</language>
</langUsage>
<abstract xml:lang="en">
<p>Abstract: The main results of an extensive study of the infrared emission from the nearby interstellar medium are presented. These results are used to discuss the origin of the infrared emission from the solar neigbourhood. We show that altough most of the emission comes from interstellar matter not associated with current star formation, about half of the heating of grains is provided by ultraviolet photons radiated by stars younger than few 108 yrs.</p>
</abstract>
<textClass>
<keywords scheme="Book-Subject-Collection">
<list>
<label>SUCO11651</label>
<item>
<term>Physics and Astronomy</term>
</item>
</list>
</keywords>
</textClass>
<textClass>
<keywords scheme="Book-Subject-Group">
<list>
<label>P</label>
<label>P22014</label>
<label>P22022</label>
<label>G18009</label>
<item>
<term>Physics</term>
</item>
<item>
<term>Astronomy</term>
</item>
<item>
<term>Astrophysics</term>
</item>
<item>
<term>Geophysics/Geodesy</term>
</item>
</list>
</keywords>
</textClass>
</profileDesc>
<revisionDesc>
<change when="2008-01-29">Published</change>
<change xml:id="refBibs-istex" who="#ISTEX-API" when="2016-09-22">References added</change>
</revisionDesc>
</teiHeader>
</istex:fulltextTEI>
<json:item>
<original>false</original>
<mimetype>text/plain</mimetype>
<extension>txt</extension>
<uri>https://api.istex.fr/document/3CF0C26C5FE45C42C57581429DB0F9C1537ED48A/fulltext/txt</uri>
</json:item>
</fulltext>
<metadata>
<istex:metadataXml wicri:clean="Springer, Publisher found" wicri:toSee="no header">
<istex:xmlDeclaration>version="1.0" encoding="UTF-8"</istex:xmlDeclaration>
<istex:docType PUBLIC="-//Springer-Verlag//DTD A++ V2.4//EN" URI="http://devel.springer.de/A++/V2.4/DTD/A++V2.4.dtd" name="istex:docType"></istex:docType>
<istex:document>
<Publisher>
<PublisherInfo>
<PublisherName>Springer Berlin Heidelberg</PublisherName>
<PublisherLocation>Berlin, Heidelberg</PublisherLocation>
</PublisherInfo>
<Series>
<SeriesInfo SeriesType="Series" TocLevels="0">
<SeriesID>5304</SeriesID>
<SeriesPrintISSN>0075-8450</SeriesPrintISSN>
<SeriesElectronicISSN>1616-6361</SeriesElectronicISSN>
<SeriesTitle Language="En">Lecture Notes in Physics</SeriesTitle>
<SeriesAbbreviatedTitle>Lect Notes Phys</SeriesAbbreviatedTitle>
</SeriesInfo>
<SeriesHeader>
<EditorGroup>
<Editor>
<EditorName DisplayOrder="Western">
<GivenName>H.</GivenName>
<FamilyName>Araki</FamilyName>
</EditorName>
</Editor>
<Editor>
<EditorName DisplayOrder="Western">
<GivenName>J.</GivenName>
<FamilyName>Ehlers</FamilyName>
</EditorName>
</Editor>
<Editor>
<EditorName DisplayOrder="Western">
<GivenName>K.</GivenName>
<FamilyName>Hepp</FamilyName>
</EditorName>
</Editor>
<Editor>
<EditorName DisplayOrder="Western">
<GivenName>R.</GivenName>
<FamilyName>Kippenhahn</FamilyName>
</EditorName>
</Editor>
<Editor>
<EditorName DisplayOrder="Western">
<GivenName>H.</GivenName>
<GivenName>A.</GivenName>
<FamilyName>Weidenmüller</FamilyName>
</EditorName>
</Editor>
<Editor>
<EditorName DisplayOrder="Western">
<GivenName>J.</GivenName>
<FamilyName>Wess</FamilyName>
</EditorName>
</Editor>
<Editor>
<EditorName DisplayOrder="Western">
<GivenName>J.</GivenName>
<FamilyName>Zittartz</FamilyName>
</EditorName>
</Editor>
</EditorGroup>
</SeriesHeader>
<Book Language="En">
<BookInfo BookProductType="Proceedings" ContainsESM="No" Language="En" MediaType="Book" NumberingStyle="Unnumbered" TocLevels="0">
<BookID>3-540-19052-X</BookID>
<BookTitle>Comets to Cosmology</BookTitle>
<BookSubTitle>Proceedings of the Third IRAS Conference Held at Queen Mary College, University of London July 6–10, 1987</BookSubTitle>
<BookVolumeNumber>297</BookVolumeNumber>
<BookSequenceNumber>297</BookSequenceNumber>
<BookDOI>10.1007/BFb0118781</BookDOI>
<BookTitleID>22254</BookTitleID>
<BookPrintISBN>978-3-540-19052-3</BookPrintISBN>
<BookElectronicISBN>978-3-540-39067-1</BookElectronicISBN>
<BookChapterCount>51</BookChapterCount>
<BookCopyright>
<CopyrightHolderName>Springer-Verlag</CopyrightHolderName>
<CopyrightYear>1988</CopyrightYear>
</BookCopyright>
<BookSubjectGroup>
<BookSubject Code="P" Type="Primary">Physics</BookSubject>
<BookSubject Code="P22014" Priority="1" Type="Secondary">Astronomy</BookSubject>
<BookSubject Code="P22022" Priority="2" Type="Secondary">Astrophysics</BookSubject>
<BookSubject Code="G18009" Priority="3" Type="Secondary">Geophysics/Geodesy</BookSubject>
<SubjectCollection Code="SUCO11651">Physics and Astronomy</SubjectCollection>
</BookSubjectGroup>
</BookInfo>
<BookHeader>
<EditorGroup>
<Editor>
<EditorName DisplayOrder="Western">
<GivenName>Andrew</GivenName>
<FamilyName>Lawrence</FamilyName>
</EditorName>
</Editor>
</EditorGroup>
</BookHeader>
<Chapter ID="Chap16" Language="En">
<ChapterInfo ChapterType="ReviewPaper" ContainsESM="No" NumberingStyle="Unnumbered" TocLevels="0">
<ChapterID>16</ChapterID>
<ChapterDOI>10.1007/BFb0118797</ChapterDOI>
<ChapterSequenceNumber>16</ChapterSequenceNumber>
<ChapterTitle Language="En">Infrared emission from the solar neighborhood</ChapterTitle>
<ChapterCategory>The Galaxy</ChapterCategory>
<ChapterFirstPage>122</ChapterFirstPage>
<ChapterLastPage>129</ChapterLastPage>
<ChapterCopyright>
<CopyrightHolderName>Springer-Verlag</CopyrightHolderName>
<CopyrightYear>1988</CopyrightYear>
</ChapterCopyright>
<ChapterHistory>
<OnlineDate>
<Year>2008</Year>
<Month>1</Month>
<Day>29</Day>
</OnlineDate>
</ChapterHistory>
<ChapterGrants Type="Regular">
<MetadataGrant Grant="OpenAccess"></MetadataGrant>
<AbstractGrant Grant="OpenAccess"></AbstractGrant>
<BodyPDFGrant Grant="Restricted"></BodyPDFGrant>
<BodyHTMLGrant Grant="Restricted"></BodyHTMLGrant>
<BibliographyGrant Grant="Restricted"></BibliographyGrant>
<ESMGrant Grant="Restricted"></ESMGrant>
</ChapterGrants>
<ChapterContext>
<SeriesID>5304</SeriesID>
<BookID>3-540-19052-X</BookID>
<BookTitle>Comets to Cosmology</BookTitle>
</ChapterContext>
</ChapterInfo>
<ChapterHeader>
<AuthorGroup>
<Author AffiliationIDS="Aff1">
<AuthorName DisplayOrder="Western">
<GivenName>F.</GivenName>
<FamilyName>Boulanger</FamilyName>
</AuthorName>
</Author>
<Author AffiliationIDS="Aff2">
<AuthorName DisplayOrder="Western">
<GivenName>M.</GivenName>
<FamilyName>Pérault</FamilyName>
</AuthorName>
</Author>
<Affiliation ID="Aff1">
<OrgName>IPAC, Caltech</OrgName>
<OrgAddress>
<Postbox>100-22</Postbox>
<Postcode>91125</Postcode>
<City>Pasadena</City>
<State>CA</State>
<Country>USA</Country>
</OrgAddress>
</Affiliation>
<Affiliation ID="Aff2">
<OrgName>Ecole Normale Supérieure</OrgName>
<OrgAddress>
<Street>24 rue Lhomond</Street>
<Postcode>75016</Postcode>
<City>Paris</City>
<Country>France</Country>
</OrgAddress>
</Affiliation>
</AuthorGroup>
<Abstract ID="Abs1" Language="En">
<Heading>Abstract</Heading>
<Para>The main results of an extensive study of the infrared emission from the nearby interstellar medium are presented. These results are used to discuss the origin of the infrared emission from the solar neigbourhood. We show that altough most of the emission comes from interstellar matter not associated with current star formation, about half of the heating of grains is provided by ultraviolet photons radiated by stars younger than few 10
<Superscript>8</Superscript>
yrs.</Para>
</Abstract>
</ChapterHeader>
<NoBody></NoBody>
</Chapter>
</Book>
</Series>
</Publisher>
</istex:document>
</istex:metadataXml>
<mods version="3.6">
<titleInfo lang="en">
<title>Infrared emission from the solar neighborhood</title>
</titleInfo>
<titleInfo type="alternative" contentType="CDATA" lang="en">
<title>Infrared emission from the solar neighborhood</title>
</titleInfo>
<name type="personal">
<namePart type="given">F.</namePart>
<namePart type="family">Boulanger</namePart>
<affiliation>IPAC, Caltech, 100-22, 91125, Pasadena, CA, USA</affiliation>
<role>
<roleTerm type="text">author</roleTerm>
</role>
</name>
<name type="personal">
<namePart type="given">M.</namePart>
<namePart type="family">Pérault</namePart>
<affiliation>Ecole Normale Supérieure, 24 rue Lhomond, 75016, Paris, France</affiliation>
<role>
<roleTerm type="text">author</roleTerm>
</role>
</name>
<typeOfResource>text</typeOfResource>
<genre type="conference" displayLabel="ReviewPaper"></genre>
<originInfo>
<publisher>Springer Berlin Heidelberg</publisher>
<place>
<placeTerm type="text">Berlin, Heidelberg</placeTerm>
</place>
<dateIssued encoding="w3cdtf">2008-01-29</dateIssued>
<copyrightDate encoding="w3cdtf">1988</copyrightDate>
</originInfo>
<language>
<languageTerm type="code" authority="rfc3066">en</languageTerm>
<languageTerm type="code" authority="iso639-2b">eng</languageTerm>
</language>
<physicalDescription>
<internetMediaType>text/html</internetMediaType>
</physicalDescription>
<abstract lang="en">Abstract: The main results of an extensive study of the infrared emission from the nearby interstellar medium are presented. These results are used to discuss the origin of the infrared emission from the solar neigbourhood. We show that altough most of the emission comes from interstellar matter not associated with current star formation, about half of the heating of grains is provided by ultraviolet photons radiated by stars younger than few 108 yrs.</abstract>
<relatedItem type="host">
<titleInfo>
<title>Comets to Cosmology</title>
<subTitle>Proceedings of the Third IRAS Conference Held at Queen Mary College, University of London July 6–10, 1987</subTitle>
</titleInfo>
<name type="personal">
<namePart type="given">Andrew</namePart>
<namePart type="family">Lawrence</namePart>
<role>
<roleTerm type="text">editor</roleTerm>
</role>
</name>
<genre type="book-series" displayLabel="Proceedings"></genre>
<originInfo>
<copyrightDate encoding="w3cdtf">1988</copyrightDate>
<issuance>monographic</issuance>
</originInfo>
<subject>
<genre>Book-Subject-Collection</genre>
<topic authority="SpringerSubjectCodes" authorityURI="SUCO11651">Physics and Astronomy</topic>
</subject>
<subject>
<genre>Book-Subject-Group</genre>
<topic authority="SpringerSubjectCodes" authorityURI="P">Physics</topic>
<topic authority="SpringerSubjectCodes" authorityURI="P22014">Astronomy</topic>
<topic authority="SpringerSubjectCodes" authorityURI="P22022">Astrophysics</topic>
<topic authority="SpringerSubjectCodes" authorityURI="G18009">Geophysics/Geodesy</topic>
</subject>
<identifier type="DOI">10.1007/BFb0118781</identifier>
<identifier type="ISBN">978-3-540-19052-3</identifier>
<identifier type="eISBN">978-3-540-39067-1</identifier>
<identifier type="ISSN">0075-8450</identifier>
<identifier type="eISSN">1616-6361</identifier>
<identifier type="BookTitleID">22254</identifier>
<identifier type="BookID">3-540-19052-X</identifier>
<identifier type="BookChapterCount">51</identifier>
<identifier type="BookVolumeNumber">297</identifier>
<identifier type="BookSequenceNumber">297</identifier>
<part>
<date>1988</date>
<detail type="volume">
<number>297</number>
<caption>vol.</caption>
</detail>
<extent unit="pages">
<start>122</start>
<end>129</end>
</extent>
</part>
<recordInfo>
<recordOrigin>Springer-Verlag, 1988</recordOrigin>
</recordInfo>
</relatedItem>
<relatedItem type="series">
<titleInfo>
<title>Lecture Notes in Physics</title>
</titleInfo>
<name type="personal">
<namePart type="given">H.</namePart>
<namePart type="family">Araki</namePart>
<role>
<roleTerm type="text">editor</roleTerm>
</role>
</name>
<name type="personal">
<namePart type="given">J.</namePart>
<namePart type="family">Ehlers</namePart>
<role>
<roleTerm type="text">editor</roleTerm>
</role>
</name>
<name type="personal">
<namePart type="given">K.</namePart>
<namePart type="family">Hepp</namePart>
<role>
<roleTerm type="text">editor</roleTerm>
</role>
</name>
<name type="personal">
<namePart type="given">R.</namePart>
<namePart type="family">Kippenhahn</namePart>
<role>
<roleTerm type="text">editor</roleTerm>
</role>
</name>
<name type="personal">
<namePart type="given">H.</namePart>
<namePart type="given">A.</namePart>
<namePart type="family">Weidenmüller</namePart>
<role>
<roleTerm type="text">editor</roleTerm>
</role>
</name>
<name type="personal">
<namePart type="given">J.</namePart>
<namePart type="family">Wess</namePart>
<role>
<roleTerm type="text">editor</roleTerm>
</role>
</name>
<name type="personal">
<namePart type="given">J.</namePart>
<namePart type="family">Zittartz</namePart>
<role>
<roleTerm type="text">editor</roleTerm>
</role>
</name>
<originInfo>
<copyrightDate encoding="w3cdtf">1988</copyrightDate>
<issuance>serial</issuance>
</originInfo>
<identifier type="ISSN">0075-8450</identifier>
<identifier type="eISSN">1616-6361</identifier>
<identifier type="SeriesID">5304</identifier>
<recordInfo>
<recordOrigin>Springer-Verlag, 1988</recordOrigin>
</recordInfo>
</relatedItem>
<identifier type="istex">3CF0C26C5FE45C42C57581429DB0F9C1537ED48A</identifier>
<identifier type="DOI">10.1007/BFb0118797</identifier>
<identifier type="ChapterID">16</identifier>
<identifier type="ChapterID">Chap16</identifier>
<accessCondition type="use and reproduction" contentType="copyright">Springer-Verlag, 1988</accessCondition>
<recordInfo>
<recordContentSource>SPRINGER</recordContentSource>
<recordOrigin>Springer-Verlag, 1988</recordOrigin>
</recordInfo>
</mods>
</metadata>
<enrichments>
<json:item>
<type>multicat</type>
<uri>https://api.istex.fr/document/3CF0C26C5FE45C42C57581429DB0F9C1537ED48A/enrichments/multicat</uri>
</json:item>
<istex:refBibTEI uri="https://api.istex.fr/document/3CF0C26C5FE45C42C57581429DB0F9C1537ED48A/enrichments/refBib">
<teiHeader></teiHeader>
<text>
<front></front>
<body></body>
<back>
<listBibl>
<biblStruct xml:id="b0">
<monogr>
<title></title>
<author>
<persName>
<forename type="first">F</forename>
<surname>Boulanger</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">R</forename>
<forename type="middle">S</forename>
<surname>Cohen</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">M</forename>
<surname>Gaida</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">I</forename>
<surname>Grenier</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">M</forename>
<surname>Koprucu</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">L~</forename>
<forename type="middle">J</forename>
<surname>Maddalena</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">P</forename>
<surname>Thaddeus</surname>
</persName>
</author>
<imprint></imprint>
</monogr>
<note>and. Ungerechts, H. 1988, In preparation</note>
</biblStruct>
<biblStruct xml:id="b1">
<analytic>
<title></title>
<author>
<persName>
<forename type="first">T</forename>
<forename type="middle">M</forename>
<surname>Dame</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">R</forename>
<forename type="middle">S</forename>
<surname>Ungerechts</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">R</forename>
<forename type="middle">S</forename>
<surname>Cohen</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">E</forename>
<surname>De Geus</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">I</forename>
<forename type="middle">A</forename>
<surname>Grenier</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">J</forename>
<surname>May</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">D</forename>
<forename type="middle">C</forename>
<surname>Murphy</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">L</forename>
<forename type="middle">A</forename>
<surname>Nyman</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">Thaddeus</forename>
<forename type="middle">P</forename>
</persName>
</author>
<author>
<persName>
<forename type="first">Houck</forename>
</persName>
</author>
</analytic>
<monogr>
<title level="j">Ap. J. J.R. Ap. J</title>
<imprint>
<publisher>In press Hacking</publisher>
<publisher>In press Hacking</publisher>
<biblScope unit="page">311</biblScope>
<date type="published" when="1987"></date>
</imprint>
</monogr>
<note>Suppl. . 63</note>
</biblStruct>
<biblStruct xml:id="b2">
<analytic>
<title></title>
<author>
<persName>
<forename type="first">D</forename>
<surname>Leisawitz</surname>
</persName>
</author>
</analytic>
<monogr>
<title level="m">Star Formation in Galaxies</title>
<editor>C.J. Lonsdale Persson Lockman, F. J</editor>
<imprint>
<date type="published" when="1984"></date>
<biblScope unit="page">90</biblScope>
</imprint>
</monogr>
</biblStruct>
<biblStruct xml:id="b3">
<analytic>
<title></title>
<author>
<persName>
<surname>Magnani</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">L</forename>
<surname>Blitz</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">L</forename>
<surname>Mundy</surname>
</persName>
</author>
</analytic>
<monogr>
<title level="j">Ap. J</title>
<imprint>
<biblScope unit="volume">295</biblScope>
<biblScope unit="page">402</biblScope>
<date type="published" when="1985"></date>
</imprint>
</monogr>
</biblStruct>
<biblStruct xml:id="b4">
<analytic>
<title></title>
<author>
<persName>
<forename type="first">J</forename>
<forename type="middle">S</forename>
<surname>Mathis</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">P</forename>
<forename type="middle">G</forename>
<surname>Mezger</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">N</forename>
<surname>Panagia</surname>
</persName>
</author>
</analytic>
<monogr>
<title level="j">Astr. Ap</title>
<imprint>
<biblScope unit="volume">128</biblScope>
<biblScope unit="page">212</biblScope>
<date type="published" when="1983"></date>
</imprint>
</monogr>
</biblStruct>
<biblStruct xml:id="b5">
<analytic>
<title></title>
<author>
<persName>
<forename type="first">R</forename>
<forename type="middle">J</forename>
<surname>Reynolds</surname>
</persName>
</author>
</analytic>
<monogr>
<title level="j">Ap. J</title>
<imprint>
<biblScope unit="volume">282</biblScope>
<biblScope unit="page">191</biblScope>
<date type="published" when="1984"></date>
</imprint>
</monogr>
</biblStruct>
<biblStruct xml:id="b6">
<monogr>
<title></title>
<author>
<persName>
<forename type="first">A</forename>
<forename type="middle">A</forename>
<surname>Stark</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">J</forename>
<surname>Bally</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">R</forename>
<forename type="middle">A</forename>
<surname>Linke</surname>
</persName>
</author>
<author>
<persName>
<forename type="first">C</forename>
<surname>Heiles</surname>
</persName>
</author>
<imprint>
<date type="published" when="1987"></date>
</imprint>
</monogr>
<note>In. preparation. Viallefond, F.</note>
</biblStruct>
</listBibl>
</back>
</text>
</istex:refBibTEI>
<json:item>
<type>refBibs</type>
<uri>https://api.istex.fr/document/3CF0C26C5FE45C42C57581429DB0F9C1537ED48A/enrichments/refBibs</uri>
</json:item>
</enrichments>
</istex>
</record>

Pour manipuler ce document sous Unix (Dilib)

EXPLOR_STEP=$WICRI_ROOT/Wicri/Amerique/explor/CaltechV1/Data/Main/Corpus
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 000327 | SxmlIndent | more

Ou

HfdSelect -h $EXPLOR_AREA/Data/Main/Corpus/biblio.hfd -nk 000327 | SxmlIndent | more

Pour mettre un lien sur cette page dans le réseau Wicri

{{Explor lien
   |wiki=    Wicri/Amerique
   |area=    CaltechV1
   |flux=    Main
   |étape=   Corpus
   |type=    RBID
   |clé=     ISTEX:3CF0C26C5FE45C42C57581429DB0F9C1537ED48A
   |texte=   Infrared emission from the solar neighborhood
}}

Wicri

This area was generated with Dilib version V0.6.32.
Data generation: Sat Nov 11 11:37:59 2017. Site generation: Mon Feb 12 16:27:53 2024