Meet the family - the catalog of known hot subdwarf stars

被引:16
作者
Geier, Stephan [1 ]
Ostensen, Roy H. [2 ]
Nemeth, Peter [3 ,4 ]
Heber, Ulrich [3 ,4 ]
Fusillo, Nicola P. Gentile [5 ]
Gansicke, Boris T. [5 ]
Telting, John H. [6 ]
Green, Elizabeth M. [7 ]
Schaffenroth, Johannes [3 ,4 ]
机构
[1] Eberhard Karls Univ Tubingen, Inst Astron & Astrophys, Kepler Ctr Astro & Particle Phys, Sand 1, D-72076 Tubingen, Germany
[2] Missouri State Univ, Dept Phys Astron & Mat Sci, Springfield, MO 65804 USA
[3] Friedrich Alexander Univ Erlangen Nuremberg, Dr Karl Remeis Observ, Sternwartstr 7, D-96049 Bamberg, Germany
[4] Friedrich Alexander Univ Erlangen Nuremberg, ECAP, Astron Inst, Sternwartstr 7, D-96049 Bamberg, Germany
[5] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England
[6] Nord Opt Telescope, Rambla Jose Ana Fernandez Perez 7, E-38711 Brena Baja, Spain
[7] Univ Arizona, Steward Observ, 933 North Cherry Ave, Tucson, AZ 85721 USA
关键词
stars: subdwarfs; stars: horizontal branch; catalogs; SDB STARS; SPECTRAL-ANALYSIS; 3D KINEMATICS; WHITE-DWARFS; SPY PROJECT; POPULATIONS; SELECTION; IA;
D O I
10.1515/astro-2017-0432
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In preparation for the upcoming all-sky data releases of the Gaia mission, we compiled a catalog of known hot subdwarf stars and candidates drawn from the literature and yet unpublished databases. The catalog contains 5613 unique sources and provides multi-band photometry from the ultraviolet to the far infrared, ground based proper motions, classifications based on spectroscopy and colors, published atmospheric parameters, radial velocities and light curve variability information. Using several different techniques, we removed outliers and misclassified objects. By matching this catalog with astrometric and photometric data from the Gaia mission, we will develop selection criteria to construct a homogeneous, magnitude-limited all-sky catalog of hot subdwarf stars based on Gaia data. As first application of the catalog data, we present the quantitative spectral analysis of 280 sdB and sdOB stars from the Sloan Digital Sky Survey Data Release 7. Combining our derived parameters with state-of-the-art proper motions, we performed a full kinematic analysis of our sample. This allowed us to separate the first significantly large sample of 78 sdBs and sdOBs belonging to the Galactic halo. Comparing the properties of hot subdwarfs from the disk and the halo with hot subdwarf samples from the globular clusters omega Cen and NGC 2808, we found the fraction of intermediate He-sdOBs in the field halo population to be significantly smaller than in the globular clusters.
引用
收藏
页码:164 / 168
页数:5
相关论文
共 32 条
[1]   Studying the populations of our Galaxy using the kinematics of sdB stars [J].
Altmann, M ;
Edelmann, H ;
de Boer, KS .
ASTRONOMY & ASTROPHYSICS, 2004, 414 (01) :181-201
[2]  
[Anonymous], A A
[3]  
deBoer KS, 1997, ASTRON ASTROPHYS, V327, P577
[4]   ULTRAVIOLET-RADIATION FROM EVOLVED STELLAR POPULATIONS .1. MODELS [J].
DORMAN, B ;
ROOD, RT ;
OCONNELL, RW .
ASTROPHYSICAL JOURNAL, 1993, 419 (02) :596-614
[5]   Spectral analysis of sdB stars from the Hamburg Quasar Survey [J].
Edelmann, H ;
Heber, U ;
Hagen, HJ ;
Lemke, M ;
Dreizler, S ;
Napiwotzki, R ;
Engels, D .
ASTRONOMY & ASTROPHYSICS, 2003, 400 (03) :939-950
[6]  
Geier S., 2017, A A, V600, P50
[7]  
Geier S., 2015, A A, V577, P26
[8]  
Heber U, 2000, ASTRON ASTROPHYS, V363, P198
[9]   Hot Subluminous Stars [J].
Heber, U. .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2016, 128 (966)
[10]  
HEBER U, 1986, ASTRON ASTROPHYS, V155, P33