Chemically tagging the Hyades Supercluster
نویسندگان
چکیده
منابع مشابه
New Photometry of the Hyades
71 Tauri (= BS 1394 = vB 141 = V777 Tau) is a rapidly rotating, F0 IV–V member of the Hyades cluster. It is the second brightest X-ray source in the cluster, after V471 Tauri, and an intensely bright coronal EUV source (Stern et al. 1995). It is a lunar occultation binary, but the secondary star (estimated by Peterson et al. 1981 to be a G4 V star in possibly a 53 day orbit) has never been seen...
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ژورنال
عنوان ژورنال: Astronomy & Astrophysics
سال: 2012
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361/201117506