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http://hdl.handle.net/2248/67| Title: | NU Centauri: A New Beta Cephei Star |
| Authors: | Rajamohan, R |
| Keywords: | Spctroscopic Binaries Variable Stars |
| Issue Date: | 1977 |
| Publisher: | Indian Institute of Astrophysics, Bangalore |
| Citation: | Kodaikanal Observatory Bulletins Series A, Vol. 2, pp. 6-9 |
| Abstract: | Spectroscopic observations of the single-lined binary, NU Centauri during the years 1968-1972 were utilised to derive fresh orbital elements of this system. The measured radial velocities indicate that the primary component is a Beta Cephei type with a period of 0.1750 days |
| URI: | http://hdl.handle.net/2248/67 |
| ISSN: | 0374-3632 |
| Appears in Collections: | IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 ) |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| NU Centauri: A New Beta Cephei Star.pdf | 130.67 kB | Adobe PDF | View/Open |
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