AustralieFrV1, Istex, Curation, bibRecord, 001205

Magnetic fields and differential rotation on the pre‐main sequence – III. The early‐G star HD 106506

Identifieur interne : 001205 ( Istex/Curation ); précédent : 001204; suivant : 001206

Magnetic fields and differential rotation on the pre‐main sequence – III. The early‐G star HD 106506

Auteurs : I. A. Waite [Australie] ; S. C. Marsden [Australie] ; B. D. Carter [Australie] ; R. Hart [Australie] ; J. Donati [France] ; J. C. Ramírez Vélez [France] ; M. Semel [France] ; N. Dunstone

Source :

Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2011-05-21.

RBID : ISTEX:5F0E3BB048B7422F59BB90663213AD4170CD9AC9

English descriptors

Abstract

We present the photometry and spectropolarimetry of the pre‐main‐sequence star HD 106506. A photometric rotational period of ∼1.416 ± 0.133 d has been derived using observations at Mount Kent Observatory (MKO). Spectropolarimetric data obtained with the 3.9‐m Anglo‐Australian Telescope (AAT) were used to derive spot occupancy and magnetic maps of the star through the technique of Zeeman Doppler imaging (ZDI). The resulting brightness maps indicate that HD 106506 displays photospheric spots at all latitudes including a predominant polar spot. Azimuthal and radial magnetic images of this star have been derived, and a significant azimuthal magnetic field is indicated, in line with other active young stars. A solar‐like differential rotation law was incorporated into the imaging process. Using Stokes I information the equatorial rotation rate, Ωeq, was found to be 4.54 ± 0.01 rad d−1, with a photospheric shear δΩ of 0.21+0.02−0.03 rad d−1. This equates to an equatorial rotation period of ∼1.39 ± 0.01 d, with the equatorial region lapping the poles every ∼ 30+5−3 d. Using the magnetic features, the equatorial rotation rate, Ωeq, was found to be 4.51 ± 0.01 rad d−1, with a photospheric shear δΩ of 0.24 ± 0.03 rad d−1. This differential rotation is approximately four times that observed on the Sun.

Url:

https://api.istex.fr/document/5F0E3BB048B7422F59BB90663213AD4170CD9AC9/fulltext/pdf

DOI: 10.1111/j.1365-2966.2011.18366.x

Links toward previous steps (curation, corpus...)

to stream Istex, to step Corpus: Pour aller vers cette notice dans l'étape Curation :001205

Links to Exploration step

ISTEX:5F0E3BB048B7422F59BB90663213AD4170CD9AC9

Curation

No country items

N. Dunstone

<affiliation><mods:affiliation>SUPA, School of Physics and Astronomy, University of St Andrews, St Andrews KY16 9SS</mods:affiliation>
<wicri:noCountry code="subField">9SS</wicri:noCountry>
</affiliation>

Le document en format XML

<record><TEI wicri:istexFullTextTei="biblStruct"><teiHeader><fileDesc><titleStmt><title xml:lang="en">Magnetic fields and differential rotation on the pre‐main sequence – III. The early‐G star HD 106506</title>
<author><name sortKey="Waite, I A" sort="Waite, I A" uniqKey="Waite I" first="I. A." last="Waite">I. A. Waite</name>
<affiliation wicri:level="1"><mods:affiliation>Faculty of Sciences, University of Southern Queensland, Toowoomba 4350, Australia</mods:affiliation>
<country xml:lang="fr">Australie</country>
<wicri:regionArea>Faculty of Sciences, University of Southern Queensland, Toowoomba 4350</wicri:regionArea>
</affiliation>
<affiliation wicri:level="1"><mods:affiliation>E-mail: waite@usq.edu.au</mods:affiliation>
<country wicri:rule="url">Australie</country>
</affiliation>
</author>
<author><name sortKey="Marsden, S C" sort="Marsden, S C" uniqKey="Marsden S" first="S. C." last="Marsden">S. C. Marsden</name>
<affiliation wicri:level="1"><mods:affiliation>Australian Astronomical Observatory, PO Box 296, Epping, Sydney 1710, Australia</mods:affiliation>
<country xml:lang="fr">Australie</country>
<wicri:regionArea>Australian Astronomical Observatory, PO Box 296, Epping, Sydney 1710</wicri:regionArea>
</affiliation>
<affiliation wicri:level="1"><mods:affiliation>Centre for Astronomy, School of Engineering and Physical Sciences, James Cook University, Townsville 4811, Australia</mods:affiliation>
<country xml:lang="fr">Australie</country>
<wicri:regionArea>Centre for Astronomy, School of Engineering and Physical Sciences, James Cook University, Townsville 4811</wicri:regionArea>
</affiliation>
</author>
<author><name sortKey="Carter, B D" sort="Carter, B D" uniqKey="Carter B" first="B. D." last="Carter">B. D. Carter</name>
<affiliation wicri:level="1"><mods:affiliation>Faculty of Sciences, University of Southern Queensland, Toowoomba 4350, Australia</mods:affiliation>
<country xml:lang="fr">Australie</country>
<wicri:regionArea>Faculty of Sciences, University of Southern Queensland, Toowoomba 4350</wicri:regionArea>
</affiliation>
</author>
<author><name sortKey="Hart, R" sort="Hart, R" uniqKey="Hart R" first="R." last="Hart">R. Hart</name>
<affiliation wicri:level="1"><mods:affiliation>Faculty of Sciences, University of Southern Queensland, Toowoomba 4350, Australia</mods:affiliation>
<country xml:lang="fr">Australie</country>
<wicri:regionArea>Faculty of Sciences, University of Southern Queensland, Toowoomba 4350</wicri:regionArea>
</affiliation>
</author>
<author><name sortKey="Donati, J" sort="Donati, J" uniqKey="Donati J" first="J." last="Donati">J. Donati</name>
<affiliation wicri:level="1"><mods:affiliation>LATT‐UMR 5572, CNRS & Univ. de Toulouse, 14 Av. E. Belin, F‐31400 Toulouse, France</mods:affiliation>
<country xml:lang="fr">France</country>
<wicri:regionArea>LATT‐UMR 5572, CNRS & Univ. de Toulouse, 14 Av. E. Belin, F‐31400 Toulouse</wicri:regionArea>
</affiliation>
</author>
<author><name sortKey="Ramirez Velez, J C" sort="Ramirez Velez, J C" uniqKey="Ramirez Velez J" first="J. C." last="Ramírez Vélez">J. C. Ramírez Vélez</name>
<affiliation wicri:level="1"><mods:affiliation>LESIA, Observatoire de Paris‐Meudon, F‐92195 Meudon Cedex, France</mods:affiliation>
<country xml:lang="fr">France</country>
<wicri:regionArea>LESIA, Observatoire de Paris‐Meudon, F‐92195 Meudon Cedex</wicri:regionArea>
</affiliation>
<affiliation><mods:affiliation>Instituto de Astronomia, Universidad Nacional Autónoma de México, 04510 Coyoacon, México D.F</mods:affiliation>
<wicri:noCountry code="subField">D.F</wicri:noCountry>
</affiliation>
</author>
<author><name sortKey="Semel, M" sort="Semel, M" uniqKey="Semel M" first="M." last="Semel">M. Semel</name>
<affiliation wicri:level="1"><mods:affiliation>LATT‐UMR 5572, CNRS & Univ. de Toulouse, 14 Av. E. Belin, F‐31400 Toulouse, France</mods:affiliation>
<country xml:lang="fr">France</country>
<wicri:regionArea>LATT‐UMR 5572, CNRS & Univ. de Toulouse, 14 Av. E. Belin, F‐31400 Toulouse</wicri:regionArea>
</affiliation>
</author>
<author><name sortKey="Dunstone, N" sort="Dunstone, N" uniqKey="Dunstone N" first="N." last="Dunstone">N. Dunstone</name>
<affiliation><mods:affiliation>SUPA, School of Physics and Astronomy, University of St Andrews, St Andrews KY16 9SS</mods:affiliation>
<wicri:noCountry code="subField">9SS</wicri:noCountry>
</affiliation>
</author>
</titleStmt>
<publicationStmt><idno type="wicri:source">ISTEX</idno>
<idno type="RBID">ISTEX:5F0E3BB048B7422F59BB90663213AD4170CD9AC9</idno>
<date when="2011" year="2011">2011</date>
<idno type="doi">10.1111/j.1365-2966.2011.18366.x</idno>
<idno type="url">https://api.istex.fr/document/5F0E3BB048B7422F59BB90663213AD4170CD9AC9/fulltext/pdf</idno>
<idno type="wicri:Area/Istex/Corpus">001205</idno>
<idno type="wicri:explorRef" wicri:stream="Istex" wicri:step="Corpus" wicri:corpus="ISTEX">001205</idno>
<idno type="wicri:Area/Istex/Curation">001205</idno>
</publicationStmt>
<sourceDesc><biblStruct><analytic><title level="a" type="main">Magnetic fields and differential rotation on the pre‐main sequence – III. The early‐G star HD 106506</title>
<author><name sortKey="Waite, I A" sort="Waite, I A" uniqKey="Waite I" first="I. A." last="Waite">I. A. Waite</name>
<affiliation wicri:level="1"><mods:affiliation>Faculty of Sciences, University of Southern Queensland, Toowoomba 4350, Australia</mods:affiliation>
<country xml:lang="fr">Australie</country>
<wicri:regionArea>Faculty of Sciences, University of Southern Queensland, Toowoomba 4350</wicri:regionArea>
</affiliation>
<affiliation wicri:level="1"><mods:affiliation>E-mail: waite@usq.edu.au</mods:affiliation>
<country wicri:rule="url">Australie</country>
</affiliation>
</author>
<author><name sortKey="Marsden, S C" sort="Marsden, S C" uniqKey="Marsden S" first="S. C." last="Marsden">S. C. Marsden</name>
<affiliation wicri:level="1"><mods:affiliation>Australian Astronomical Observatory, PO Box 296, Epping, Sydney 1710, Australia</mods:affiliation>
<country xml:lang="fr">Australie</country>
<wicri:regionArea>Australian Astronomical Observatory, PO Box 296, Epping, Sydney 1710</wicri:regionArea>
</affiliation>
<affiliation wicri:level="1"><mods:affiliation>Centre for Astronomy, School of Engineering and Physical Sciences, James Cook University, Townsville 4811, Australia</mods:affiliation>
<country xml:lang="fr">Australie</country>
<wicri:regionArea>Centre for Astronomy, School of Engineering and Physical Sciences, James Cook University, Townsville 4811</wicri:regionArea>
</affiliation>
</author>
<author><name sortKey="Carter, B D" sort="Carter, B D" uniqKey="Carter B" first="B. D." last="Carter">B. D. Carter</name>
<affiliation wicri:level="1"><mods:affiliation>Faculty of Sciences, University of Southern Queensland, Toowoomba 4350, Australia</mods:affiliation>
<country xml:lang="fr">Australie</country>
<wicri:regionArea>Faculty of Sciences, University of Southern Queensland, Toowoomba 4350</wicri:regionArea>
</affiliation>
</author>
<author><name sortKey="Hart, R" sort="Hart, R" uniqKey="Hart R" first="R." last="Hart">R. Hart</name>
<affiliation wicri:level="1"><mods:affiliation>Faculty of Sciences, University of Southern Queensland, Toowoomba 4350, Australia</mods:affiliation>
<country xml:lang="fr">Australie</country>
<wicri:regionArea>Faculty of Sciences, University of Southern Queensland, Toowoomba 4350</wicri:regionArea>
</affiliation>
</author>
<author><name sortKey="Donati, J" sort="Donati, J" uniqKey="Donati J" first="J." last="Donati">J. Donati</name>
<affiliation wicri:level="1"><mods:affiliation>LATT‐UMR 5572, CNRS & Univ. de Toulouse, 14 Av. E. Belin, F‐31400 Toulouse, France</mods:affiliation>
<country xml:lang="fr">France</country>
<wicri:regionArea>LATT‐UMR 5572, CNRS & Univ. de Toulouse, 14 Av. E. Belin, F‐31400 Toulouse</wicri:regionArea>
</affiliation>
</author>
<author><name sortKey="Ramirez Velez, J C" sort="Ramirez Velez, J C" uniqKey="Ramirez Velez J" first="J. C." last="Ramírez Vélez">J. C. Ramírez Vélez</name>
<affiliation wicri:level="1"><mods:affiliation>LESIA, Observatoire de Paris‐Meudon, F‐92195 Meudon Cedex, France</mods:affiliation>
<country xml:lang="fr">France</country>
<wicri:regionArea>LESIA, Observatoire de Paris‐Meudon, F‐92195 Meudon Cedex</wicri:regionArea>
</affiliation>
<affiliation><mods:affiliation>Instituto de Astronomia, Universidad Nacional Autónoma de México, 04510 Coyoacon, México D.F</mods:affiliation>
</affiliation>
</author>
<author><name sortKey="Semel, M" sort="Semel, M" uniqKey="Semel M" first="M." last="Semel">M. Semel</name>
<affiliation wicri:level="1"><mods:affiliation>LATT‐UMR 5572, CNRS & Univ. de Toulouse, 14 Av. E. Belin, F‐31400 Toulouse, France</mods:affiliation>
<country xml:lang="fr">France</country>
<wicri:regionArea>LATT‐UMR 5572, CNRS & Univ. de Toulouse, 14 Av. E. Belin, F‐31400 Toulouse</wicri:regionArea>
</affiliation>
</author>
<author><name sortKey="Dunstone, N" sort="Dunstone, N" uniqKey="Dunstone N" first="N." last="Dunstone">N. Dunstone</name>
<affiliation><mods:affiliation>SUPA, School of Physics and Astronomy, University of St Andrews, St Andrews KY16 9SS</mods:affiliation>
<wicri:noCountry code="subField">9SS</wicri:noCountry>
</affiliation>
</author>
</analytic>
<monogr></monogr>
<series><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title>
<title level="j" type="alt">MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY</title>
<idno type="ISSN">0035-8711</idno>
<idno type="eISSN">1365-2966</idno>
<imprint><biblScope unit="vol">413</biblScope>
<biblScope unit="issue">3</biblScope>
<biblScope unit="page" from="1949">1949</biblScope>
<biblScope unit="page" to="1960">1960</biblScope>
<biblScope unit="page-count">12</biblScope>
<publisher>Blackwell Publishing Ltd</publisher>
<pubPlace>Oxford, UK</pubPlace>
<date type="published" when="2011-05-21">2011-05-21</date>
</imprint>
<idno type="ISSN">0035-8711</idno>
</series>
</biblStruct>
</sourceDesc>
<seriesStmt><idno type="ISSN">0035-8711</idno>
</seriesStmt>
</fileDesc>
<profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Aperture size</term>
<term>April</term>
<term>Average spot occupancy</term>
<term>Azimuthal</term>
<term>Azimuthal ring</term>
<term>Bolometric corrections</term>
<term>Brighter stars</term>
<term>Brightness image</term>
<term>Cameron</term>
<term>Chromospheric features</term>
<term>Collier</term>
<term>Collier cameron</term>
<term>Comparison stars</term>
<term>Convective</term>
<term>Convective zone</term>
<term>Differential rotation</term>
<term>Differential rotation parameters</term>
<term>Discrete fourier</term>
<term>Donati</term>
<term>Donati collier cameron</term>
<term>Donati landstreet</term>
<term>Donati rees</term>
<term>Donati semel</term>
<term>Doppler</term>
<term>Doppler imaging</term>
<term>Doppler imaging process</term>
<term>Dynamic spectra</term>
<term>Dynamic spectrum</term>
<term>Effective temperature</term>
<term>Eld</term>
<term>Equatorial</term>
<term>Equatorial rotation period</term>
<term>Equatorial rotation rate</term>
<term>Error bars</term>
<term>Error ellipses</term>
<term>Fractional spottedness</term>
<term>Fresnel rhomb</term>
<term>Graphical purposes</term>
<term>Higher latitude features</term>
<term>Image reconstruction</term>
<term>Imaging</term>
<term>Imaging process</term>
<term>Inclination angle</term>
<term>Instrumental polarization signals</term>
<term>Jeffers</term>
<term>Jeffers donati</term>
<term>Kent observatory</term>
<term>Latitude</term>
<term>Latitude parallels</term>
<term>Light curve</term>
<term>Lling factor</term>
<term>Louisville telescope</term>
<term>Lower latitude features</term>
<term>Magnetic dynamo</term>
<term>Magnetic energy</term>
<term>Magnetic features</term>
<term>Magnetic images</term>
<term>Magnetic maps</term>
<term>Marsden</term>
<term>Minimization techniques</term>
<term>Minimum value</term>
<term>Mnras</term>
<term>Modelled lines</term>
<term>Monthly notices</term>
<term>Nightly master</term>
<term>Other stars</term>
<term>Photcal package</term>
<term>Photometric</term>
<term>Photometric data</term>
<term>Photometric observations</term>
<term>Photometry</term>
<term>Photospheric</term>
<term>Photospheric shear</term>
<term>Polar projections</term>
<term>Polar spots</term>
<term>Poloidal</term>
<term>Poloidal component</term>
<term>Program stars</term>
<term>Radial ticks</term>
<term>Radial velocity</term>
<term>Rotation</term>
<term>Rotation rate</term>
<term>Rotational</term>
<term>Rotational phases</term>
<term>Rotational shear</term>
<term>Rotational velocity</term>
<term>Semel</term>
<term>Sempol polarimeter</term>
<term>Small sample</term>
<term>Solar value</term>
<term>Southern queensland</term>
<term>Spectral line</term>
<term>Spectropolarimetric data</term>
<term>Spectropolarimetric observations</term>
<term>Spectroscopic</term>
<term>Spectroscopic data</term>
<term>Spectroscopy extracts</term>
<term>Spot coverage</term>
<term>Spot features</term>
<term>Spot occupancy</term>
<term>Spot temperature</term>
<term>Standard stars</term>
<term>Stellar</term>
<term>Stellar latitude</term>
<term>Stellar parameters</term>
<term>Stellar surface</term>
<term>Stokes</term>
<term>Surface temperature</term>
<term>Target star</term>
<term>Thick lines</term>
<term>Thin lines</term>
<term>Toroidal</term>
<term>Toroidal component</term>
<term>Unruh collier cameron</term>
<term>Waite</term>
<term>Young stars</term>
<term>Zeeman doppler imaging</term>
</keywords>
<keywords scheme="Teeft" xml:lang="en"><term>Aperture size</term>
<term>April</term>
<term>Average spot occupancy</term>
<term>Azimuthal</term>
<term>Azimuthal ring</term>
<term>Bolometric corrections</term>
<term>Brighter stars</term>
<term>Brightness image</term>
<term>Cameron</term>
<term>Chromospheric features</term>
<term>Collier</term>
<term>Collier cameron</term>
<term>Comparison stars</term>
<term>Convective</term>
<term>Convective zone</term>
<term>Differential rotation</term>
<term>Differential rotation parameters</term>
<term>Discrete fourier</term>
<term>Donati</term>
<term>Donati collier cameron</term>
<term>Donati landstreet</term>
<term>Donati rees</term>
<term>Donati semel</term>
<term>Doppler</term>
<term>Doppler imaging</term>
<term>Doppler imaging process</term>
<term>Dynamic spectra</term>
<term>Dynamic spectrum</term>
<term>Effective temperature</term>
<term>Eld</term>
<term>Equatorial</term>
<term>Equatorial rotation period</term>
<term>Equatorial rotation rate</term>
<term>Error bars</term>
<term>Error ellipses</term>
<term>Fractional spottedness</term>
<term>Fresnel rhomb</term>
<term>Graphical purposes</term>
<term>Higher latitude features</term>
<term>Image reconstruction</term>
<term>Imaging</term>
<term>Imaging process</term>
<term>Inclination angle</term>
<term>Instrumental polarization signals</term>
<term>Jeffers</term>
<term>Jeffers donati</term>
<term>Kent observatory</term>
<term>Latitude</term>
<term>Latitude parallels</term>
<term>Light curve</term>
<term>Lling factor</term>
<term>Louisville telescope</term>
<term>Lower latitude features</term>
<term>Magnetic dynamo</term>
<term>Magnetic energy</term>
<term>Magnetic features</term>
<term>Magnetic images</term>
<term>Magnetic maps</term>
<term>Marsden</term>
<term>Minimization techniques</term>
<term>Minimum value</term>
<term>Mnras</term>
<term>Modelled lines</term>
<term>Monthly notices</term>
<term>Nightly master</term>
<term>Other stars</term>
<term>Photcal package</term>
<term>Photometric</term>
<term>Photometric data</term>
<term>Photometric observations</term>
<term>Photometry</term>
<term>Photospheric</term>
<term>Photospheric shear</term>
<term>Polar projections</term>
<term>Polar spots</term>
<term>Poloidal</term>
<term>Poloidal component</term>
<term>Program stars</term>
<term>Radial ticks</term>
<term>Radial velocity</term>
<term>Rotation</term>
<term>Rotation rate</term>
<term>Rotational</term>
<term>Rotational phases</term>
<term>Rotational shear</term>
<term>Rotational velocity</term>
<term>Semel</term>
<term>Sempol polarimeter</term>
<term>Small sample</term>
<term>Solar value</term>
<term>Southern queensland</term>
<term>Spectral line</term>
<term>Spectropolarimetric data</term>
<term>Spectropolarimetric observations</term>
<term>Spectroscopic</term>
<term>Spectroscopic data</term>
<term>Spectroscopy extracts</term>
<term>Spot coverage</term>
<term>Spot features</term>
<term>Spot occupancy</term>
<term>Spot temperature</term>
<term>Standard stars</term>
<term>Stellar</term>
<term>Stellar latitude</term>
<term>Stellar parameters</term>
<term>Stellar surface</term>
<term>Stokes</term>
<term>Surface temperature</term>
<term>Target star</term>
<term>Thick lines</term>
<term>Thin lines</term>
<term>Toroidal</term>
<term>Toroidal component</term>
<term>Unruh collier cameron</term>
<term>Waite</term>
<term>Young stars</term>
<term>Zeeman doppler imaging</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front><div type="abstract" xml:lang="en">We present the photometry and spectropolarimetry of the pre‐main‐sequence star HD 106506. A photometric rotational period of ∼1.416 ± 0.133 d has been derived using observations at Mount Kent Observatory (MKO). Spectropolarimetric data obtained with the 3.9‐m Anglo‐Australian Telescope (AAT) were used to derive spot occupancy and magnetic maps of the star through the technique of Zeeman Doppler imaging (ZDI). The resulting brightness maps indicate that HD 106506 displays photospheric spots at all latitudes including a predominant polar spot. Azimuthal and radial magnetic images of this star have been derived, and a significant azimuthal magnetic field is indicated, in line with other active young stars. A solar‐like differential rotation law was incorporated into the imaging process. Using Stokes I information the equatorial rotation rate, Ωeq, was found to be 4.54 ± 0.01 rad d−1, with a photospheric shear δΩ of 0.21+0.02−0.03 rad d−1. This equates to an equatorial rotation period of ∼1.39 ± 0.01 d, with the equatorial region lapping the poles every ∼ 30+5−3 d. Using the magnetic features, the equatorial rotation rate, Ωeq, was found to be 4.51 ± 0.01 rad d−1, with a photospheric shear δΩ of 0.24 ± 0.03 rad d−1. This differential rotation is approximately four times that observed on the Sun.</div>
</front>
</TEI>
</record>

Pour manipuler ce document sous Unix (Dilib)

EXPLOR_STEP=$WICRI_ROOT/Wicri/Asie/explor/AustralieFrV1/Data/Istex/Curation

HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 001205 | SxmlIndent | more

HfdSelect -h $EXPLOR_AREA/Data/Istex/Curation/biblio.hfd -nk 001205 | SxmlIndent | more

Pour mettre un lien sur cette page dans le réseau Wicri

{{Explor lien
   |wiki=    Wicri/Asie
   |area=    AustralieFrV1
   |flux=    Istex
   |étape=   Curation
   |type=    RBID
   |clé=     ISTEX:5F0E3BB048B7422F59BB90663213AD4170CD9AC9
   |texte=   Magnetic fields and differential rotation on the pre‐main sequence – III. The early‐G star HD 106506
}}

This area was generated with Dilib version V0.6.33.
Data generation: Tue Dec 5 10:43:12 2017. Site generation: Tue Mar 5 14:07:20 2024

	Serveur d'exploration sur les relations entre la France et l'Australie
	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.

Serveur d'exploration sur les relations entre la France et l'Australie

Magnetic fields and differential rotation on the pre‐main sequence – III. The early‐G star HD 106506

Magnetic fields and differential rotation on the pre‐main sequence – III. The early‐G star HD 106506

Source :

English descriptors

Abstract

Links toward previous steps (curation, corpus...)

Links to Exploration step

Curation

No country items

Le document en format XML

Pour manipuler ce document sous Unix (Dilib)

Pour mettre un lien sur cette page dans le réseau Wicri