Suspected VV Cephei stars in the Large Magellanic Cloud
Journal Article
·
· Astrophys. J., v. 201, no. 2, pp. 347-349
OSTI ID:4098911
Twelve stars in the Large Magellanic Cloud show both hydrogen emission and TiO absorption features in the red and/or infrared. Five of these are known to be composite, apparently combining an M supergiant and a luminous blue component, and are probably VV Cephei stars. The remaining stars are suspected to be of a similar character. (AIP)
- Research Organization:
- Warner and Swasey Observatory, Case Western Reserve University
- NSA Number:
- NSA-33-018183
- OSTI ID:
- 4098911
- Journal Information:
- Astrophys. J., v. 201, no. 2, pp. 347-349, Journal Name: Astrophys. J., v. 201, no. 2, pp. 347-349; ISSN ASJOA
- Country of Publication:
- United States
- Language:
- English
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