New CH Carbon Stars Found in the DFBS

G. Kostandyan (1) , K. S. Gigoyan (1) , Alain Sarkissian (2) , Mustapha Meftah (2) , F. Zamkotsian (3)

1 BAO - V.A. Ambartsumian Byurakan Astrophysical Observatory
2 STRATO - LATMOS
3 LAM - Laboratoire d'Astrophysique de Marseille

In this paper, we discuss the nature of three new carbon © stars discovered in the Digitized First Byurakan Survey (DFBS). The three stars show early-type spectra in the DFBS. To better characterize these objects, medium-resolution CCD spectra were obtained. These stars show spectral features typical to CH-giants

Domains: Sciences of the Universe [physics]; Astrophysics [astro-ph]; Solar and Stellar Astrophysics [astro-ph.SR]

G. Kostandyan, K. S. Gigoyan, Alain Sarkissian, Mustapha Meftah, F. Zamkotsian. New CH Carbon Stars Found in the DFBS. Astrophysics, 2017, 60 (2), pp.300 - 303. ⟨10.1007/s10511-017-9483-8⟩. ⟨insu-01562571⟩