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A search for new members of the β Pictoris, Tucana–Horologium and ε Cha moving groups in the RAVE data base

Identifieur interne : 001688 ( Istex/Corpus ); précédent : 001687; suivant : 001689

A search for new members of the β Pictoris, Tucana–Horologium and ε Cha moving groups in the RAVE data base

Auteurs : L. L. Kiss ; A. Mo R ; T. Szalai ; J. Kovács ; D. Bayliss ; G. F. Gilmore ; O. Bienaymé ; J. Binney ; J. Bland-Hawthorn ; R. Campbell ; K. C. Freeman ; J. P. Fulbright ; B. K. Gibson ; E. K. Grebel ; A. Helmi ; U. Munari ; J. F. Navarro ; Q. A. Parker ; W. Reid ; G. M. Seabroke ; A. Siebert ; A. Siviero ; M. Steinmetz ; F. G. Watson ; M. Williams ; R. F. G. Wyse ; T. Zwitter

Source :

RBID : ISTEX:79385BF20223A06B064A45F2C597FC144059BE98

English descriptors

Abstract

We report on the discovery of new members of nearby young moving groups, exploiting the full power of combining the Radial Velocity Experiment (RAVE) survey with several stellar age diagnostic methods and follow‐up high‐resolution optical spectroscopy. The results include the identification of one new and five likely members of the β Pictoris moving group, ranging from spectral types F9 to M4 with the majority being M dwarfs, one K7 likely member of the ε Cha group and two stars in the Tucana–Horologium association. Based on the positive identifications, we foreshadow a great potential of the RAVE data base in progressing towards a full census of young moving groups in the solar neighbourhood.

Url:
DOI: 10.1111/j.1365-2966.2010.17660.x

Links to Exploration step

ISTEX:79385BF20223A06B064A45F2C597FC144059BE98

Le document en format XML

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<name sortKey="Bland Awthorn, J" sort="Bland Awthorn, J" uniqKey="Bland Awthorn J" first="J." last="Bland-Hawthorn">J. Bland-Hawthorn</name>
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<name sortKey="Campbell, R" sort="Campbell, R" uniqKey="Campbell R" first="R." last="Campbell">R. Campbell</name>
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<p>We report on the discovery of new members of nearby young moving groups, exploiting the full power of combining the Radial Velocity Experiment (RAVE) survey with several stellar age diagnostic methods and follow‐up high‐resolution optical spectroscopy. The results include the identification of one new and five likely members of the β Pictoris moving group, ranging from spectral types F9 to M4 with the majority being M dwarfs, one K7 likely member of the ε Cha group and two stars in the Tucana–Horologium association. Based on the positive identifications, we foreshadow a great potential of the RAVE data base in progressing towards a full census of young moving groups in the solar neighbourhood.</p>
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<p>We report on the discovery of new members of nearby young moving groups, exploiting the full power of combining the Radial Velocity Experiment (RAVE) survey with several stellar age diagnostic methods and follow‐up high‐resolution optical spectroscopy. The results include the identification of one new and five likely members of the β Pictoris moving group, ranging from spectral types F9 to M4 with the majority being M dwarfs, one K7 likely member of the ε Cha group and two stars in the Tucana–Horologium association. Based on the positive identifications, we foreshadow a great potential of the RAVE data base in progressing towards a full census of young moving groups in the solar neighbourhood.</p>
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<namePart type="given">L. L.</namePart>
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<namePart type="given">G. F.</namePart>
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<namePart type="given">O.</namePart>
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<namePart type="given">K. C.</namePart>
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<namePart type="given">G. M.</namePart>
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<abstract lang="en">We report on the discovery of new members of nearby young moving groups, exploiting the full power of combining the Radial Velocity Experiment (RAVE) survey with several stellar age diagnostic methods and follow‐up high‐resolution optical spectroscopy. The results include the identification of one new and five likely members of the β Pictoris moving group, ranging from spectral types F9 to M4 with the majority being M dwarfs, one K7 likely member of the ε Cha group and two stars in the Tucana–Horologium association. Based on the positive identifications, we foreshadow a great potential of the RAVE data base in progressing towards a full census of young moving groups in the solar neighbourhood.</abstract>
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