Gravitational lensing
Identifieur interne : 000689 ( Main/Exploration ); précédent : 000688; suivant : 000690Gravitational lensing
Auteurs : R. D. Blandford [États-Unis]Source :
- Nuclear Physics B (Proceedings Supplements) [ 0920-5632 ] ; 1996.
Abstract
One of the most promising uses of extragalactic gravitational lenses is as probes of the distribution of dark matter in the universe. Some recent results and the prospects for future measurements of dark matter distributions in the halos of individual galaxies, associated with rich clusters of galaxies, distributed inhomogeneously as large scale structure on ~ 1–100 Mpc scales and contributing to the overall mean density of the universe on the Hubble scale itself, are briefly reviewed.
Url:
DOI: 10.1016/S0920-5632(96)00489-6
Affiliations:
Links toward previous steps (curation, corpus...)
Le document en format XML
<record><TEI wicri:istexFullTextTei="biblStruct"><teiHeader><fileDesc><titleStmt><title xml:lang="en">Gravitational lensing</title><author><name sortKey="Blandford, R D" sort="Blandford, R D" uniqKey="Blandford R" first="R. D." last="Blandford">R. D. Blandford</name></author></titleStmt><publicationStmt><idno type="wicri:source">ISTEX</idno><idno type="RBID">ISTEX:44A61A09AA3391FA67356C9A4153643FCDAFA1EF</idno><date when="1996" year="1996">1996</date><idno type="doi">10.1016/S0920-5632(96)00489-6</idno><idno type="url">https://api.istex.fr/document/44A61A09AA3391FA67356C9A4153643FCDAFA1EF/fulltext/pdf</idno><idno type="wicri:Area/Main/Corpus">000290</idno><idno type="wicri:Area/Main/Curation">000290</idno><idno type="wicri:Area/Main/Exploration">000689</idno><idno type="wicri:explorRef" wicri:stream="Main" wicri:step="Exploration">000689</idno></publicationStmt><sourceDesc><biblStruct><analytic><title level="a" type="main" xml:lang="en">Gravitational lensing</title><author><name sortKey="Blandford, R D" sort="Blandford, R D" uniqKey="Blandford R" first="R. D." last="Blandford">R. D. Blandford</name><affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Theoretical Astrophysics, 130-33 Caltech, Pasadena, CA 91125</wicri:regionArea><wicri:noRegion>CA 91125</wicri:noRegion></affiliation><affiliation></affiliation></author></analytic><monogr></monogr><series><title level="j">Nuclear Physics B (Proceedings Supplements)</title><title level="j" type="abbrev">NUPHBP</title><idno type="ISSN">0920-5632</idno><imprint><publisher>ELSEVIER</publisher><date type="published" when="1996">1996</date><biblScope unit="volume">51</biblScope><biblScope unit="issue">2</biblScope><biblScope unit="page" from="101">101</biblScope><biblScope unit="page" to="106">106</biblScope></imprint><idno type="ISSN">0920-5632</idno></series><idno type="istex">44A61A09AA3391FA67356C9A4153643FCDAFA1EF</idno><idno type="DOI">10.1016/S0920-5632(96)00489-6</idno><idno type="PII">S0920-5632(96)00489-6</idno><idno type="ArticleID">96004896</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0920-5632</idno></seriesStmt></fileDesc><profileDesc><textClass></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">One of the most promising uses of extragalactic gravitational lenses is as probes of the distribution of dark matter in the universe. Some recent results and the prospects for future measurements of dark matter distributions in the halos of individual galaxies, associated with rich clusters of galaxies, distributed inhomogeneously as large scale structure on ~ 1–100 Mpc scales and contributing to the overall mean density of the universe on the Hubble scale itself, are briefly reviewed.</div></front></TEI><affiliations><list><country><li>États-Unis</li></country></list><tree><country name="États-Unis"><noRegion><name sortKey="Blandford, R D" sort="Blandford, R D" uniqKey="Blandford R" first="R. D." last="Blandford">R. D. Blandford</name></noRegion></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
EXPLOR_STEP=$WICRI_ROOT/Wicri/Amerique/explor/CaltechV1/Data/Main/Exploration
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 000689 | SxmlIndent | more
Ou
HfdSelect -h $EXPLOR_AREA/Data/Main/Exploration/biblio.hfd -nk 000689 | SxmlIndent | more
Pour mettre un lien sur cette page dans le réseau Wicri
{{Explor lien
|wiki= Wicri/Amerique
|area= CaltechV1
|flux= Main
|étape= Exploration
|type= RBID
|clé= ISTEX:44A61A09AA3391FA67356C9A4153643FCDAFA1EF
|texte= Gravitational lensing
}}
| This area was generated with Dilib version V0.6.32. |  |