V5485 Sagittarii: A Possible Symbiotic Star Exhibiting Ellipsoidal Variation Evidence as Orbital Signature

Details V5485 Sagittarii: A Possible Symbiotic Star Exhibiting Ellipsoidal Variation Evidence as Orbital Signature V5485 Sagittarii: A Possible Symbiotic Star Exhibiting Ellipsoidal Variation Evidence as Orbital Signature

2010-02-26

arxiv.org/abs/1002.4970v2

Greaves, J., (2009), Peremennye Zvezdy Prilozhenie, vol.9, no. 13

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

withdrawn

Scientific paper

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.

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