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The variable star SBS 0150+339

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Plates from the Second Byurakan Survey reveal two large increases in the brightness of this star in 1972 and 1975. Spectra of this variable have been obtained for the first time. It is not visible in plate H2133 from the Hamburg survey, which has a limiting brightness of ~18m. Our data confirm that the star is an eruptive variable, most likely of the U Gem type.

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References

  1. J. A. Stepanian, Rev. Mex. Astron. Astrof. 41, 155–368 (2005).

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  2. C. Watson, A. A. Henden, and A. Price, http://www.aavso.org/vsx/

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Authors and Affiliations

  1. V. A. Ambartsumyan Byurakan Astrophysical Observatory, Byurakan, Armenia

    L. K. Erastova

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  1. L. K. Erastova
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Correspondence to L. K. Erastova.

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Translated from Astrofizika, Vol. 54, No. 1, pp. 167–169 (February 2011).

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Erastova, L.K. The variable star SBS 0150+339. Astrophysics 54, 143–145 (2011). https://doi.org/10.1007/s10511-011-9166-9

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  • DOI: https://doi.org/10.1007/s10511-011-9166-9

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