SBS 0802+529: A New Variable Star from the Second Byurakan Survey
Chavushyan V., Erastova L., Tovmassian G. and 2 more
Open Astronomy · 2012
doi:10.1515/astro-2017-0379 (opens in a new tab)
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Abstract
A new emission line star was discovered on the plates of the Second Byurakan Survey (SBS). the follow up spectroscopy demonstrated that the object had a spectrum dominated by a late-type giant star with superposed hydrogen emission lines. the object resembles a pulsating Mira, but the amplitude of variability and a rapid UV variability are quite unusual for a single star, and we tentatively classify the object as a symbiotic star.
Abstract licence: CC BY
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