V5485 Sagittarii: A Possible Symbiotic Star Exhibiting Ellipsoidal Variation Evidence as Orbital Signature
classification
🌌 astro-ph.SR
keywords
ellipsoidalorbitalsagittariistarsymbioticv5485variationcandidate
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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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