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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
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
3 LAM - Laboratoire d'Astrophysique de Marseille
Abstract : 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
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https://hal-insu.archives-ouvertes.fr/insu-01562571
Contributor : Catherine Cardon <>
Submitted on : Saturday, July 15, 2017 - 6:02:41 PM
Last modification on : Friday, January 10, 2020 - 3:42:31 PM

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INSU | CNRS | OSU-INSTITUT-PYTHEAS | LAM | UNIV-AMU | UPMC | LATMOS | UVSQ | UNIV-PARIS-SACLAY | SORBONNE-UNIVERSITE | SU-SCIENCES

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

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