Discovery of new nearby L and late-M dwarfs at low Galactic latitude from the DENIS data base
Identifieur interne : 003299 ( PascalFrancis/Checkpoint ); précédent : 003298; suivant : 003300Discovery of new nearby L and late-M dwarfs at low Galactic latitude from the DENIS data base
Auteurs : N. Phan-Bao [Taïwan, États-Unis] ; M. S. Bessell [Australie] ; E. L. Martin [États-Unis, Espagne] ; G. Simon [France] ; J. Borsenberger [France] ; R. Tata [États-Unis] ; J. Guibert [France] ; F. Crifo [France] ; T. Forveille [France] ; X. Delfosse [France] ; J. Lim [Taïwan] ; B. De Batz [France]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2008.
Descripteurs français
- Pascal (Inist)
English descriptors
- KwdEn :
Abstract
We report on new nearby L and late-M dwarfs (dphot ≤ 30 pc) discovered in our search for nearby ultracool dwarfs (I-J ≥ 3.0, later than M8.0) at low Galactic latitude (|b| < 15°) over 4800 deg2 in the Deep Near Infrared Survey of the Southern Sky (DENIS) data base. We used late-M (≥ M8.0), L and T dwarfs with accurate trigonometric parallaxes to calibrate the Mj versus I-J colour-luminosity relation. The resulting photometric distances have standard errors of ∼ 15 per cent, which we used to select candidates dphot ≤ 30 pc. We measured proper motions from multi-epoch images found in the public archives ALADIN, DSS, 2MASS and DENIS, with at least three distinct epochs and time baselines of 10-21 yr. We then used a maximum reduced proper motion cut-off to select 28 candidates as ultracool dwarfs (M8.0-L8.0) and to reject one as a distant red star. No T dwarf candidates were found in this search, which required an object to be detected in all three DENIS bands. Our low-resolution optical spectra confirmed that 26 were indeed ultracool dwarfs, with spectral types from M8.0 to L5.5. Two contaminants and one rejected by the maximum reduced proper motion cut-off were all reddened F-K main sequence stars. 20 of these 26 ultracool dwarfs are new nearby ultracool dwarf members, three L dwarfs within 15 pc with one L3.5 at only ∼ 10 pc. We determine a stellar density of ϕJ cor = (1.64 ± 0.46) x 10-3 dwarfs pc-3 mag-1 over 11.1 ≤ MJ ≤ 13.1 based on this sample of M8-L3.5 ultracool dwarfs. Our ultracool dwarf density value is in good agreement with the measurement by Cruz et al. of the ultracool dwarf density at high Galactic latitude.
Affiliations:
- Australie, Espagne, France, Taïwan, États-Unis
- Auvergne-Rhône-Alpes, Rhône-Alpes, Île-de-France
- Grenoble, Paris
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Phan-Bao</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Institute of Astronomy and Astrophysics, Academia Sinica, PO Box 23-141</s1><s2>Taipei 106</s2><s3>TWN</s3><sZ>1 aut.</sZ><sZ>11 aut.</sZ></inist:fA14><country>Taïwan</country><wicri:noRegion>Taipei 106</wicri:noRegion></affiliation><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>University of Central Florida, Department of Physics, PO Box 162385</s1><s2>Orlando, FL 32816-2385</s2><s3>USA</s3><sZ>1 aut.</sZ><sZ>3 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>États-Unis</country><wicri:noRegion>Orlando, FL 32816-2385</wicri:noRegion></affiliation></author><author><name sortKey="Bessell, M S" sort="Bessell, M S" uniqKey="Bessell M" first="M. S." last="Bessell">M. S. 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Crifo</name><affiliation wicri:level="1"><inist:fA14 i1="05"><s1>GEPI, Observatoire de Paris, 5 place J. Janssen</s1><s2>92195 Meudon</s2><s3>FRA</s3><sZ>4 aut.</sZ><sZ>8 aut.</sZ><sZ>12 aut.</sZ></inist:fA14><country>France</country><wicri:noRegion>92195 Meudon</wicri:noRegion><wicri:noRegion>5 place J. Janssen</wicri:noRegion><wicri:noRegion>92195 Meudon</wicri:noRegion></affiliation></author><author><name sortKey="Forveille, T" sort="Forveille, T" uniqKey="Forveille T" first="T." last="Forveille">T. Forveille</name><affiliation wicri:level="1"><inist:fA14 i1="08"><s1>Laboratoire d'Astrophysique de Grenoble, Université J. Fourier, BP 53</s1><s2>38041 Grenoble</s2><s3>FRA</s3><sZ>9 aut.</sZ><sZ>10 aut.</sZ></inist:fA14><country>France</country><wicri:noRegion>38041 Grenoble</wicri:noRegion><placeName><settlement type="city">Grenoble</settlement><region type="region" nuts="2">Auvergne-Rhône-Alpes</region><region type="old region" nuts="2">Rhône-Alpes</region></placeName></affiliation></author><author><name sortKey="Delfosse, X" sort="Delfosse, X" uniqKey="Delfosse X" first="X." last="Delfosse">X. Delfosse</name><affiliation wicri:level="1"><inist:fA14 i1="08"><s1>Laboratoire d'Astrophysique de Grenoble, Université J. Fourier, BP 53</s1><s2>38041 Grenoble</s2><s3>FRA</s3><sZ>9 aut.</sZ><sZ>10 aut.</sZ></inist:fA14><country>France</country><wicri:noRegion>38041 Grenoble</wicri:noRegion><placeName><settlement type="city">Grenoble</settlement><region type="region" nuts="2">Auvergne-Rhône-Alpes</region><region type="old region" nuts="2">Rhône-Alpes</region></placeName></affiliation></author><author><name sortKey="Lim, J" sort="Lim, J" uniqKey="Lim J" first="J." last="Lim">J. Lim</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Institute of Astronomy and Astrophysics, Academia Sinica, PO Box 23-141</s1><s2>Taipei 106</s2><s3>TWN</s3><sZ>1 aut.</sZ><sZ>11 aut.</sZ></inist:fA14><country>Taïwan</country><wicri:noRegion>Taipei 106</wicri:noRegion></affiliation></author><author><name sortKey="De Batz, B" sort="De Batz, B" uniqKey="De Batz B" first="B." last="De Batz">B. De Batz</name><affiliation wicri:level="1"><inist:fA14 i1="05"><s1>GEPI, Observatoire de Paris, 5 place J. Janssen</s1><s2>92195 Meudon</s2><s3>FRA</s3><sZ>4 aut.</sZ><sZ>8 aut.</sZ><sZ>12 aut.</sZ></inist:fA14><country>France</country><wicri:noRegion>92195 Meudon</wicri:noRegion><wicri:noRegion>5 place J. 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Phan-Bao</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Institute of Astronomy and Astrophysics, Academia Sinica, PO Box 23-141</s1><s2>Taipei 106</s2><s3>TWN</s3><sZ>1 aut.</sZ><sZ>11 aut.</sZ></inist:fA14><country>Taïwan</country><wicri:noRegion>Taipei 106</wicri:noRegion></affiliation><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>University of Central Florida, Department of Physics, PO Box 162385</s1><s2>Orlando, FL 32816-2385</s2><s3>USA</s3><sZ>1 aut.</sZ><sZ>3 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>États-Unis</country><wicri:noRegion>Orlando, FL 32816-2385</wicri:noRegion></affiliation></author><author><name sortKey="Bessell, M S" sort="Bessell, M S" uniqKey="Bessell M" first="M. S." last="Bessell">M. S. Bessell</name><affiliation wicri:level="1"><inist:fA14 i1="03"><s1>Research School of Astronomy and Astrophysics, Australian National University, Cotter Rd</s1><s2>Weston, ACT 2611</s2><s3>AUS</s3><sZ>2 aut.</sZ></inist:fA14><country>Australie</country><wicri:noRegion>Weston, ACT 2611</wicri:noRegion></affiliation></author><author><name sortKey="Martin, E L" sort="Martin, E L" uniqKey="Martin E" first="E. L." last="Martin">E. L. Martin</name><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>University of Central Florida, Department of Physics, PO Box 162385</s1><s2>Orlando, FL 32816-2385</s2><s3>USA</s3><sZ>1 aut.</sZ><sZ>3 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>États-Unis</country><wicri:noRegion>Orlando, FL 32816-2385</wicri:noRegion></affiliation><affiliation wicri:level="1"><inist:fA14 i1="04"><s1>Institute de Astrofisica de Canarias, C/ Via Ldctea s/n</s1><s2>38200 La Laguna, Tenerife</s2><s3>ESP</s3><sZ>3 aut.</sZ></inist:fA14><country>Espagne</country><wicri:noRegion>38200 La Laguna, Tenerife</wicri:noRegion></affiliation></author><author><name sortKey="Simon, G" sort="Simon, G" uniqKey="Simon G" first="G." last="Simon">G. Simon</name><affiliation wicri:level="1"><inist:fA14 i1="05"><s1>GEPI, Observatoire de Paris, 5 place J. Janssen</s1><s2>92195 Meudon</s2><s3>FRA</s3><sZ>4 aut.</sZ><sZ>8 aut.</sZ><sZ>12 aut.</sZ></inist:fA14><country>France</country><wicri:noRegion>92195 Meudon</wicri:noRegion><wicri:noRegion>5 place J. Janssen</wicri:noRegion><wicri:noRegion>92195 Meudon</wicri:noRegion></affiliation></author><author><name sortKey="Borsenberger, J" sort="Borsenberger, J" uniqKey="Borsenberger J" first="J." last="Borsenberger">J. Borsenberger</name><affiliation wicri:level="1"><inist:fA14 i1="06"><s1>LESIA, Observatoire de Paris, 5 place J. Janssen</s1><s2>92195 Meudon</s2><s3>FRA</s3><sZ>5 aut.</sZ></inist:fA14><country>France</country><wicri:noRegion>92195 Meudon</wicri:noRegion><wicri:noRegion>5 place J. Janssen</wicri:noRegion><wicri:noRegion>92195 Meudon</wicri:noRegion></affiliation></author><author><name sortKey="Tata, R" sort="Tata, R" uniqKey="Tata R" first="R." last="Tata">R. Tata</name><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>University of Central Florida, Department of Physics, PO Box 162385</s1><s2>Orlando, FL 32816-2385</s2><s3>USA</s3><sZ>1 aut.</sZ><sZ>3 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>États-Unis</country><wicri:noRegion>Orlando, FL 32816-2385</wicri:noRegion></affiliation></author><author><name sortKey="Guibert, J" sort="Guibert, J" uniqKey="Guibert J" first="J." last="Guibert">J. Guibert</name><affiliation wicri:level="1"><inist:fA14 i1="07"><s1>Centre d'Analyse des Images, GEPI, Observatoire de Paris, 61 avenue de l'Observatoire</s1><s2>75014 Paris</s2><s3>FRA</s3><sZ>7 aut.</sZ></inist:fA14><country>France</country><wicri:noRegion>75014 Paris</wicri:noRegion><placeName><settlement type="city">Paris</settlement><region type="région" nuts="2">Île-de-France</region></placeName></affiliation></author><author><name sortKey="Crifo, F" sort="Crifo, F" uniqKey="Crifo F" first="F." last="Crifo">F. Crifo</name><affiliation wicri:level="1"><inist:fA14 i1="05"><s1>GEPI, Observatoire de Paris, 5 place J. Janssen</s1><s2>92195 Meudon</s2><s3>FRA</s3><sZ>4 aut.</sZ><sZ>8 aut.</sZ><sZ>12 aut.</sZ></inist:fA14><country>France</country><wicri:noRegion>92195 Meudon</wicri:noRegion><wicri:noRegion>5 place J. Janssen</wicri:noRegion><wicri:noRegion>92195 Meudon</wicri:noRegion></affiliation></author><author><name sortKey="Forveille, T" sort="Forveille, T" uniqKey="Forveille T" first="T." last="Forveille">T. Forveille</name><affiliation wicri:level="1"><inist:fA14 i1="08"><s1>Laboratoire d'Astrophysique de Grenoble, Université J. Fourier, BP 53</s1><s2>38041 Grenoble</s2><s3>FRA</s3><sZ>9 aut.</sZ><sZ>10 aut.</sZ></inist:fA14><country>France</country><wicri:noRegion>38041 Grenoble</wicri:noRegion><placeName><settlement type="city">Grenoble</settlement><region type="region" nuts="2">Auvergne-Rhône-Alpes</region><region type="old region" nuts="2">Rhône-Alpes</region></placeName></affiliation></author><author><name sortKey="Delfosse, X" sort="Delfosse, X" uniqKey="Delfosse X" first="X." last="Delfosse">X. Delfosse</name><affiliation wicri:level="1"><inist:fA14 i1="08"><s1>Laboratoire d'Astrophysique de Grenoble, Université J. Fourier, BP 53</s1><s2>38041 Grenoble</s2><s3>FRA</s3><sZ>9 aut.</sZ><sZ>10 aut.</sZ></inist:fA14><country>France</country><wicri:noRegion>38041 Grenoble</wicri:noRegion><placeName><settlement type="city">Grenoble</settlement><region type="region" nuts="2">Auvergne-Rhône-Alpes</region><region type="old region" nuts="2">Rhône-Alpes</region></placeName></affiliation></author><author><name sortKey="Lim, J" sort="Lim, J" uniqKey="Lim J" first="J." last="Lim">J. Lim</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Institute of Astronomy and Astrophysics, Academia Sinica, PO Box 23-141</s1><s2>Taipei 106</s2><s3>TWN</s3><sZ>1 aut.</sZ><sZ>11 aut.</sZ></inist:fA14><country>Taïwan</country><wicri:noRegion>Taipei 106</wicri:noRegion></affiliation></author><author><name sortKey="De Batz, B" sort="De Batz, B" uniqKey="De Batz B" first="B." last="De Batz">B. De Batz</name><affiliation wicri:level="1"><inist:fA14 i1="05"><s1>GEPI, Observatoire de Paris, 5 place J. Janssen</s1><s2>92195 Meudon</s2><s3>FRA</s3><sZ>4 aut.</sZ><sZ>8 aut.</sZ><sZ>12 aut.</sZ></inist:fA14><country>France</country><wicri:noRegion>92195 Meudon</wicri:noRegion><wicri:noRegion>5 place J. Janssen</wicri:noRegion><wicri:noRegion>92195 Meudon</wicri:noRegion></affiliation></author></analytic><series><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="abbreviated">Mon. Not. R. Astron. Soc.</title><idno type="ISSN">0035-8711</idno><imprint><date when="2008">2008</date></imprint></series></biblStruct></sourceDesc><seriesStmt><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="abbreviated">Mon. Not. R. Astron. Soc.</title><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Brown dwarf stars</term><term>Color</term><term>High density</term><term>Infrared surveys</term><term>K stars</term><term>Low-mass stars</term><term>Luminosity</term><term>Luminosity function</term><term>Main sequence stars</term><term>Mass function</term><term>Multiple image</term><term>Optical spectrum</term><term>Proper motion</term><term>Red stars</term><term>Solar neighborhood</term><term>Spectral type</term><term>Stellar mass</term></keywords><keywords scheme="Pascal" xml:lang="fr"><term>Etude IR</term><term>Couleur</term><term>Luminosité</term><term>Mouvement propre</term><term>Image multiple</term><term>Etoile rouge</term><term>Spectre optique</term><term>Type spectral</term><term>Etoile K</term><term>Etoile séquence principale</term><term>Densité élevée</term><term>Etoile faible masse</term><term>Naine brune</term><term>Masse stellaire</term><term>Fonction luminosité</term><term>Fonction masse</term><term>Voisinage solaire</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">We report on new nearby L and late-M dwarfs (d<sub>phot</sub> ≤ 30 pc) discovered in our search for nearby ultracool dwarfs (I-J ≥ 3.0, later than M8.0) at low Galactic latitude (|b| < 15°) over 4800 deg<sup>2</sup> in the Deep Near Infrared Survey of the Southern Sky (DENIS) data base. We used late-M (≥ M8.0), L and T dwarfs with accurate trigonometric parallaxes to calibrate the Mj versus I-J colour-luminosity relation. The resulting photometric distances have standard errors of ∼ 15 per cent, which we used to select candidates d<sub>phot</sub> ≤ 30 pc. We measured proper motions from multi-epoch images found in the public archives ALADIN, DSS, 2MASS and DENIS, with at least three distinct epochs and time baselines of 10-21 yr. We then used a maximum reduced proper motion cut-off to select 28 candidates as ultracool dwarfs (M8.0-L8.0) and to reject one as a distant red star. No T dwarf candidates were found in this search, which required an object to be detected in all three DENIS bands. Our low-resolution optical spectra confirmed that 26 were indeed ultracool dwarfs, with spectral types from M8.0 to L5.5. Two contaminants and one rejected by the maximum reduced proper motion cut-off were all reddened F-K main sequence stars. 20 of these 26 ultracool dwarfs are new nearby ultracool dwarf members, three L dwarfs within 15 pc with one L3.5 at only ∼ 10 pc. We determine a stellar density of ϕ<sub>J</sub> <sub>cor</sub> = (1.64 ± 0.46) x 10<sup>-3</sup> dwarfs pc<sup>-3</sup> mag<sup>-1</sup> over 11.1 ≤ M<sub>J</sub> ≤ 13.1 based on this sample of M8-L3.5 ultracool dwarfs. Our ultracool dwarf density value is in good agreement with the measurement by Cruz et al. of the ultracool dwarf density at high Galactic latitude.</div></front></TEI><inist><standard h6="B"><pA><fA01 i1="01" i2="1"><s0>0035-8711</s0></fA01><fA02 i1="01"><s0>MNRAA4</s0></fA02><fA03 i2="1"><s0>Mon. Not. R. Astron. Soc.</s0></fA03><fA05><s2>383</s2></fA05><fA06><s2>3</s2></fA06><fA08 i1="01" i2="1" l="ENG"><s1>Discovery of new nearby L and late-M dwarfs at low Galactic latitude from the DENIS data base</s1></fA08><fA11 i1="01" i2="1"><s1>PHAN-BAO (N.)</s1></fA11><fA11 i1="02" i2="1"><s1>BESSELL (M. S.)</s1></fA11><fA11 i1="03" i2="1"><s1>MARTIN (E. L.)</s1></fA11><fA11 i1="04" i2="1"><s1>SIMON (G.)</s1></fA11><fA11 i1="05" i2="1"><s1>BORSENBERGER (J.)</s1></fA11><fA11 i1="06" i2="1"><s1>TATA (R.)</s1></fA11><fA11 i1="07" i2="1"><s1>GUIBERT (J.)</s1></fA11><fA11 i1="08" i2="1"><s1>CRIFO (F.)</s1></fA11><fA11 i1="09" i2="1"><s1>FORVEILLE (T.)</s1></fA11><fA11 i1="10" i2="1"><s1>DELFOSSE (X.)</s1></fA11><fA11 i1="11" i2="1"><s1>LIM (J.)</s1></fA11><fA11 i1="12" i2="1"><s1>DE BATZ (B.)</s1></fA11><fA14 i1="01"><s1>Institute of Astronomy and Astrophysics, Academia Sinica, PO Box 23-141</s1><s2>Taipei 106</s2><s3>TWN</s3><sZ>1 aut.</sZ><sZ>11 aut.</sZ></fA14><fA14 i1="02"><s1>University of Central Florida, Department of Physics, PO Box 162385</s1><s2>Orlando, FL 32816-2385</s2><s3>USA</s3><sZ>1 aut.</sZ><sZ>3 aut.</sZ><sZ>6 aut.</sZ></fA14><fA14 i1="03"><s1>Research School of Astronomy and Astrophysics, Australian National University, Cotter Rd</s1><s2>Weston, ACT 2611</s2><s3>AUS</s3><sZ>2 aut.</sZ></fA14><fA14 i1="04"><s1>Institute de Astrofisica de Canarias, C/ Via Ldctea s/n</s1><s2>38200 La Laguna, Tenerife</s2><s3>ESP</s3><sZ>3 aut.</sZ></fA14><fA14 i1="05"><s1>GEPI, Observatoire de Paris, 5 place J. Janssen</s1><s2>92195 Meudon</s2><s3>FRA</s3><sZ>4 aut.</sZ><sZ>8 aut.</sZ><sZ>12 aut.</sZ></fA14><fA14 i1="06"><s1>LESIA, Observatoire de Paris, 5 place J. Janssen</s1><s2>92195 Meudon</s2><s3>FRA</s3><sZ>5 aut.</sZ></fA14><fA14 i1="07"><s1>Centre d'Analyse des Images, GEPI, Observatoire de Paris, 61 avenue de l'Observatoire</s1><s2>75014 Paris</s2><s3>FRA</s3><sZ>7 aut.</sZ></fA14><fA14 i1="08"><s1>Laboratoire d'Astrophysique de Grenoble, Université J. Fourier, BP 53</s1><s2>38041 Grenoble</s2><s3>FRA</s3><sZ>9 aut.</sZ><sZ>10 aut.</sZ></fA14><fA20><s1>831-844</s1></fA20><fA21><s1>2008</s1></fA21><fA23 i1="01"><s0>ENG</s0></fA23><fA43 i1="01"><s1>INIST</s1><s2>2067</s2><s5>354000173952950020</s5></fA43><fA44><s0>0000</s0><s1>© 2008 INIST-CNRS. All rights reserved.</s1></fA44><fA45><s0>3/4 p.</s0></fA45><fA47 i1="01" i2="1"><s0>08-0084061</s0></fA47><fA60><s1>P</s1></fA60><fA61><s0>A</s0></fA61><fA64 i1="01" i2="1"><s0>Monthly Notices of the Royal Astronomical Society</s0></fA64><fA66 i1="01"><s0>GBR</s0></fA66><fC01 i1="01" l="ENG"><s0>We report on new nearby L and late-M dwarfs (d<sub>phot</sub> ≤ 30 pc) discovered in our search for nearby ultracool dwarfs (I-J ≥ 3.0, later than M8.0) at low Galactic latitude (|b| < 15°) over 4800 deg<sup>2</sup> in the Deep Near Infrared Survey of the Southern Sky (DENIS) data base. We used late-M (≥ M8.0), L and T dwarfs with accurate trigonometric parallaxes to calibrate the Mj versus I-J colour-luminosity relation. The resulting photometric distances have standard errors of ∼ 15 per cent, which we used to select candidates d<sub>phot</sub> ≤ 30 pc. We measured proper motions from multi-epoch images found in the public archives ALADIN, DSS, 2MASS and DENIS, with at least three distinct epochs and time baselines of 10-21 yr. We then used a maximum reduced proper motion cut-off to select 28 candidates as ultracool dwarfs (M8.0-L8.0) and to reject one as a distant red star. No T dwarf candidates were found in this search, which required an object to be detected in all three DENIS bands. Our low-resolution optical spectra confirmed that 26 were indeed ultracool dwarfs, with spectral types from M8.0 to L5.5. Two contaminants and one rejected by the maximum reduced proper motion cut-off were all reddened F-K main sequence stars. 20 of these 26 ultracool dwarfs are new nearby ultracool dwarf members, three L dwarfs within 15 pc with one L3.5 at only ∼ 10 pc. We determine a stellar density of ϕ<sub>J</sub> <sub>cor</sub> = (1.64 ± 0.46) x 10<sup>-3</sup> dwarfs pc<sup>-3</sup> mag<sup>-1</sup> over 11.1 ≤ M<sub>J</sub> ≤ 13.1 based on this sample of M8-L3.5 ultracool dwarfs. Our ultracool dwarf density value is in good agreement with the measurement by Cruz et al. of the ultracool dwarf density at high Galactic latitude.</s0></fC01><fC02 i1="01" i2="3"><s0>001E03</s0></fC02><fC03 i1="01" i2="3" l="FRE"><s0>Etude IR</s0><s5>26</s5></fC03><fC03 i1="01" i2="3" l="ENG"><s0>Infrared surveys</s0><s5>26</s5></fC03><fC03 i1="02" i2="3" l="FRE"><s0>Couleur</s0><s5>27</s5></fC03><fC03 i1="02" i2="3" l="ENG"><s0>Color</s0><s5>27</s5></fC03><fC03 i1="03" i2="3" l="FRE"><s0>Luminosité</s0><s5>28</s5></fC03><fC03 i1="03" i2="3" l="ENG"><s0>Luminosity</s0><s5>28</s5></fC03><fC03 i1="04" i2="3" l="FRE"><s0>Mouvement propre</s0><s5>29</s5></fC03><fC03 i1="04" i2="3" l="ENG"><s0>Proper motion</s0><s5>29</s5></fC03><fC03 i1="05" i2="X" l="FRE"><s0>Image multiple</s0><s5>30</s5></fC03><fC03 i1="05" i2="X" l="ENG"><s0>Multiple image</s0><s5>30</s5></fC03><fC03 i1="05" i2="X" l="SPA"><s0>Imagen múltiple</s0><s5>30</s5></fC03><fC03 i1="06" i2="3" l="FRE"><s0>Etoile rouge</s0><s5>31</s5></fC03><fC03 i1="06" i2="3" l="ENG"><s0>Red stars</s0><s5>31</s5></fC03><fC03 i1="07" i2="X" l="FRE"><s0>Spectre optique</s0><s5>32</s5></fC03><fC03 i1="07" i2="X" l="ENG"><s0>Optical spectrum</s0><s5>32</s5></fC03><fC03 i1="07" i2="X" l="SPA"><s0>Espectro óptico</s0><s5>32</s5></fC03><fC03 i1="08" i2="X" l="FRE"><s0>Type spectral</s0><s5>33</s5></fC03><fC03 i1="08" i2="X" l="ENG"><s0>Spectral type</s0><s5>33</s5></fC03><fC03 i1="08" i2="X" l="SPA"><s0>Tipo espectral</s0><s5>33</s5></fC03><fC03 i1="09" i2="3" l="FRE"><s0>Etoile K</s0><s5>34</s5></fC03><fC03 i1="09" i2="3" l="ENG"><s0>K stars</s0><s5>34</s5></fC03><fC03 i1="10" i2="3" l="FRE"><s0>Etoile séquence principale</s0><s5>35</s5></fC03><fC03 i1="10" i2="3" l="ENG"><s0>Main sequence stars</s0><s5>35</s5></fC03><fC03 i1="11" i2="X" l="FRE"><s0>Densité élevée</s0><s5>36</s5></fC03><fC03 i1="11" i2="X" l="ENG"><s0>High density</s0><s5>36</s5></fC03><fC03 i1="11" i2="X" l="SPA"><s0>Densidad elevada</s0><s5>36</s5></fC03><fC03 i1="12" i2="3" l="FRE"><s0>Etoile faible masse</s0><s5>37</s5></fC03><fC03 i1="12" i2="3" l="ENG"><s0>Low-mass stars</s0><s5>37</s5></fC03><fC03 i1="13" i2="3" l="FRE"><s0>Naine brune</s0><s5>38</s5></fC03><fC03 i1="13" i2="3" l="ENG"><s0>Brown dwarf stars</s0><s5>38</s5></fC03><fC03 i1="14" i2="3" l="FRE"><s0>Masse stellaire</s0><s5>39</s5></fC03><fC03 i1="14" i2="3" l="ENG"><s0>Stellar mass</s0><s5>39</s5></fC03><fC03 i1="15" i2="3" l="FRE"><s0>Fonction luminosité</s0><s5>40</s5></fC03><fC03 i1="15" i2="3" l="ENG"><s0>Luminosity function</s0><s5>40</s5></fC03><fC03 i1="16" i2="X" l="FRE"><s0>Fonction masse</s0><s5>41</s5></fC03><fC03 i1="16" i2="X" l="ENG"><s0>Mass function</s0><s5>41</s5></fC03><fC03 i1="16" i2="X" l="SPA"><s0>Función masa</s0><s5>41</s5></fC03><fC03 i1="17" i2="X" l="FRE"><s0>Voisinage solaire</s0><s5>42</s5></fC03><fC03 i1="17" i2="X" l="ENG"><s0>Solar neighborhood</s0><s5>42</s5></fC03><fC03 i1="17" i2="X" l="SPA"><s0>Vecindad solar</s0><s5>42</s5></fC03><fN21><s1>052</s1></fN21><fN44 i1="01"><s1>OTO</s1></fN44><fN82><s1>OTO</s1></fN82></pA></standard></inist><affiliations><list><country><li>Australie</li><li>Espagne</li><li>France</li><li>Taïwan</li><li>États-Unis</li></country><region><li>Auvergne-Rhône-Alpes</li><li>Rhône-Alpes</li><li>Île-de-France</li></region><settlement><li>Grenoble</li><li>Paris</li></settlement></list><tree><country name="Taïwan"><noRegion><name sortKey="Phan Bao, N" sort="Phan Bao, N" uniqKey="Phan Bao N" first="N." last="Phan-Bao">N. Phan-Bao</name></noRegion><name sortKey="Lim, J" sort="Lim, J" uniqKey="Lim J" first="J." last="Lim">J. Lim</name></country><country name="États-Unis"><noRegion><name sortKey="Phan Bao, N" sort="Phan Bao, N" uniqKey="Phan Bao N" first="N." last="Phan-Bao">N. Phan-Bao</name></noRegion><name sortKey="Martin, E L" sort="Martin, E L" uniqKey="Martin E" first="E. L." last="Martin">E. L. Martin</name><name sortKey="Tata, R" sort="Tata, R" uniqKey="Tata R" first="R." last="Tata">R. Tata</name></country><country name="Australie"><noRegion><name sortKey="Bessell, M S" sort="Bessell, M S" uniqKey="Bessell M" first="M. S." last="Bessell">M. S. Bessell</name></noRegion></country><country name="Espagne"><noRegion><name sortKey="Martin, E L" sort="Martin, E L" uniqKey="Martin E" first="E. L." last="Martin">E. L. Martin</name></noRegion></country><country name="France"><noRegion><name sortKey="Simon, G" sort="Simon, G" uniqKey="Simon G" first="G." last="Simon">G. Simon</name></noRegion><name sortKey="Borsenberger, J" sort="Borsenberger, J" uniqKey="Borsenberger J" first="J." last="Borsenberger">J. Borsenberger</name><name sortKey="Crifo, F" sort="Crifo, F" uniqKey="Crifo F" first="F." last="Crifo">F. Crifo</name><name sortKey="De Batz, B" sort="De Batz, B" uniqKey="De Batz B" first="B." last="De Batz">B. De Batz</name><name sortKey="Delfosse, X" sort="Delfosse, X" uniqKey="Delfosse X" first="X." last="Delfosse">X. Delfosse</name><name sortKey="Forveille, T" sort="Forveille, T" uniqKey="Forveille T" first="T." last="Forveille">T. Forveille</name><name sortKey="Guibert, J" sort="Guibert, J" uniqKey="Guibert J" first="J." last="Guibert">J. Guibert</name></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
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