First Byurakan Spectral Sky Survey. Stars of late spectral types. ix. -15 ≤ δ ≤-11 ° belt-Reference-Cited by-同舟云学术

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First Byurakan Spectral Sky Survey. Stars of late spectral types. ix. -15 ≤ δ ≤-11 ° belt

Published:1997-04 Issue:2 Volume:40 Page:131-139
ISSN:0571-7256
Container-title:Astrophysics
language:en
Short-container-title:Astrophysics

Author:

Abrahamyan H. V.,Gigoyan K. S.,Hambaryan V. V.,Azzopardi M.

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF03036106.pdf

Reference30 articles.

1. B. E. Markarian, V. A. Lipovetskii, and J. A. Stepanian,Astrofizika,17, 619 (1981).

2. H. V. Abrahamyan and K. S. Gigoyan,Astrofizika,36, 181 (1993).

3. K. S. Gigoyan,“Search for and investigation of late-type M and C stars on plates of the First Byurakan Spectral Sky Survey,”Dissertation, Byurakan Astrofiz. Obs., Byurakan (1994), p. 112.

4. H. V. Abrahamyan, V. V. Hambaryan, and K. S. Gigoyan,Astron. Th.,71, 891 (1994).

5. H. V. Abrahamyan and K. S. Gigoyan,Astrofizika,31, 601 (1989);32, 501 (1990);33, 317 (1990);36, 431 (1993);37, 585 (1994);38, 211 (1995).

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. A search for faint galactic carbon stars from the First Byurakan Spectral Sky Survey. I.;Astronomy & Astrophysics;2001-05

2. Commission 45: Stellar Classification: (Classification Stellaire);Transactions of the International Astronomical Union;2000

3. FBS 0102-110: A carbon star with strong CH features;Astrophysics;1999-01

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