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

被引:8
|
作者
Jimenez-Esteban, F. M. [1 ,2 ]
Caballero, J. A. [1 ]
Dorda, R. [3 ,4 ]
Miles-Paez, P. A. [3 ,5 ]
Solano, E. [1 ]
机构
[1] Ctr Astrobiol INTA CSIC, Dept Astrofis, Madrid 28691, Spain
[2] St Louis Univ, Div Sci & Engn, Madrid 28003, Spain
[3] Univ Complutense Madrid, Fac Ciencias Fis, Dept Astrofis & Ciencias Atmosfera, E-28040 Madrid, Spain
[4] Univ Alicante, Dept Fis Ingenieria Sistemas & Teoria Senal, Escuela Politecn Super, E-03080 Alicante, Spain
[5] Inst Astrofis Canarias, Tenerife 38200, Spain
来源
ASTRONOMY & ASTROPHYSICS | 2012年 / 539卷
关键词
stars: oscillations; stars: late-type; stars: chemically peculiar; virtual observatory tools; stars: peculiar; astronomical databases: miscellaneous; YZ CANIS-MINORIS; PERIOD-LUMINOSITY RELATIONS; STAR SPECTROSCOPIC SURVEY; LONG SECONDARY PERIODS; SKY AUTOMATED SURVEY; NORTH-GALACTIC POLE; FIELD M-DWARFS; GIANT STARS; SOLAR NEIGHBORHOOD; VARIABLE-STARS;
D O I
10.1051/0004-6361/201118375
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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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页数:12
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