V5485 Sagittarii: A Possible Symbiotic Star Exhibiting Ellipsoidal Variation Evidence as Orbital Signature
Abstract
MACHO project photometry shows the candidate Symbiotic Star V5485 Sagittarii's red giant component has a photometric orbital period of 270 days as evidenced by ellipsoidal variation of the lightcurve.
- Publication:
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Peremennye Zvezdy Prilozhenie
- Pub Date:
- June 2009
- DOI:
- arXiv:
- arXiv:1002.4970
- Bibcode:
- 2009PZP.....9...13G
- Keywords:
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- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- withdrawn