DM Lyrae (DM Lyr for short) is a dwarf nova in the constellation Lyra. This binary system is composed of a primary star of unknown type, and a white dwarf companion. It erupted in 1928 and 1996 and reached about magnitude 13.[1]

See also

References

  1. ^ a b c Nogami, D.; et al. (2003). "The SU UMa Nature of the Dwarf Nova, DM Lyrae". Publications of the Astronomical Society of Japan. 55 (2): 483–488. arXiv:astro-ph/0301036. Bibcode:2003PASJ...55..483N. doi:10.1093/pasj/55.2.483. S2CID 18844865.
  2. ^ a b c Downes, Ronald A.; et al. (2001). "A Catalog and Atlas of Cataclysmic Variables: The Living Edition". Publications of the Astronomical Society of the Pacific. 113 (784): 764. arXiv:astro-ph/0102302. Bibcode:2001PASP..113..764D. doi:10.1086/320802. S2CID 16285959.
  3. ^ Thorstensen, John R.; Fenton, William H. (January 2003). "Five Dwarf Novae with Orbital Periods below Two Hours". The Publications of the Astronomical Society of the Pacific. 115 (803): 37–42. arXiv:astro-ph/0209172. Bibcode:2003PASP..115...37T. doi:10.1086/345103. S2CID 119343404.
  4. ^ a b Knigge, Christian (December 2006). "The donor stars of cataclysmic variables". Monthly Notices of the Royal Astronomical Society. 373 (2): 484–502. arXiv:astro-ph/0609671. Bibcode:2006MNRAS.373..484K. doi:10.1111/j.1365-2966.2006.11096.x. S2CID 2616606.
  5. ^ "DM Lyr". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-11-15.


Allikas: https://en.wikipedia.org/wiki/DM_Lyrae
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