4.6 Article

Identification of red high proper-motion objects in Tycho-2 and 2MASS catalogues using Virtual Observatory tools

Journal

ASTRONOMY & ASTROPHYSICS
Volume 539, Issue -, Pages -

Publisher

EDP SCIENCES S A
DOI: 10.1051/0004-6361/201118375

Keywords

stars: oscillations; stars: late-type; stars: chemically peculiar; virtual observatory tools; stars: peculiar; astronomical databases: miscellaneous

Funding

  1. Spanish Ministerio de Ciencia e Innovacion
  2. Universidad Complutense de Madrid
  3. Comunidad Autonoma de Madrid [CSD2006-00070, AyA2008-00695, AyA2008-06423-C03-03, SP2009/ESP-1496]
  4. [AyA2008-02156]
  5. [RI031675]

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Aims. With available Virtual Observatory tools, we looked for new M dwarfs in the solar neighbourhood and M giants with high tangential velocities. Methods. From an all-sky cross-match between the optical Tycho-2 and the near-infrared 2MASS catalogues, we selected objects with proper motions mu > 50 mas yr(-1) and very red V-T - K-s colours. For the most interesting targets, we collected multi-wavelength photometry, constructed spectral energy distributions, estimated effective temperatures and surface gravities from fits to atmospheric models, performed time-series analysis of ASAS V-band light curves, and assigned spectral types from low-resolution spectroscopy obtained with CAFOS at the 2.2 m Calar Alto telescope. Results. We got a sample of 59 bright red high proper-motion objects, including fifty red giants, four red dwarfs, and five objects reported in this work for the first time. The five new stars have magnitudes V-T approximate to 10.8-11.3 mag, reduced proper motions midway between known dwarfs and giants, near-infrared colours typical of giants, and effective temperatures T-eff approximate to 2900-3400 K. From our time-series analysis, we discovered a long secondary period in Ruber 4 and an extremely long primary period in Ruber 6. With the CAFOS spectra, we confirmed the red giant nature of Ruber 7 and 8, the last of which seems to be one of the brightest metal-poor M giants ever identified.

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