A
visual bandlight curve for BZ Ursae Majoris. The main plot (from
AAVSO data[1]) shows several outbursts, and the inset plot (adapted from Kato et al.[2]) shows a single superoutburst in detail.
^
abcRingwald, F. A.; et al. (November 1994), "Orbital studies of the cataclysmic variables CZ Orionis, V1193 Orionis and BZ Ursae Majoris", Monthly Notices of the Royal Astronomical Society, 271 (2): 323–342,
Bibcode:
1994MNRAS.271..323R,
doi:10.1093/mnras/271.2.323.
^
abSzkody, Paula; Feinswog, Laurie (November 1988), "Infrared Light Curves of Three Novae and Three Dwarf Novae at Quiescence", Astrophysical Journal, 334: 422,
Bibcode:
1988ApJ...334..422S,
doi:
10.1086/166846.
^
abSion, Edward M. (June 2012), "White Dwarfs in Cataclysmic Variable Stars: Surface Temperatures and Evolution", Journal of Astronomy and Space Sciences, 29 (2): 169–173,
Bibcode:
2012JASS...29..169S,
doi:10.5140/JASS.2012.29.2.169.
^Neustroev, V. V.; et al. (July 2004), Tovmassian, G.; E., Sion (eds.), "New spectroscopic observations of dwarf nova BZ Ursae Majoris with extremely unusual emission lines profiles", Compact Binaries in the Galaxy and Beyond, Proceedings of the conference held 17-22 November, 2003 in La Paz, Baja California Sur, IAU Colloquium 194, Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias), vol. 20, p. 269,
Bibcode:
2004RMxAC..20..269N.
^Kukarkin, B. V.; et al. (October 1970), "57th Name-List of Variable Stars", Information Bulletin on Variable Stars, 480 (1): 1,
Bibcode:
1970IBVS..480....1K.
^Green, R. F.; Ferguson, D. H.; Liebert, J.; Schmidt, M. (June 1982), "Cataclysmic variable candidates from the Palomar Green Survey", Publications of the Astronomical Society of the Pacific, 94: 560–564,
Bibcode:
1982PASP...94..560G,
doi:
10.1086/131022,
S2CID120644760.
^Wenzel, W. (December 1982), "BZ Ursae Majoris - Missing Link Between the Dwarf Novae of U Geminorum and WZ Sagittae Type", Information Bulletin on Variable Stars, 2256 (1): 1,
Bibcode:
1982IBVS.2256....1W.
^Claudi, R.; et al. (March 1990), Green, D. W. E. (ed.), "BZ Ursae Majoris", IAU Circular, 4975 (2): 2,
Bibcode:
1990IAUC.4975....2C.
^Gänsicke, Boris T.; et al. (September 2003), "Anomalous Ultraviolet Line Flux Ratios in the Cataclysmic Variables 1RXS J232953.9+062814, CE 315, BZ Ursae Majoris, and EY Cygni, Observed with the Hubble Space Telescope Space Telescope Imaging Spectrograph", The Astrophysical Journal, 594 (1): 443–448,
arXiv:astro-ph/0305264,
Bibcode:
2003ApJ...594..443G,
doi:
10.1086/376902,
S2CID120224177.
Further reading
Sion, E. M.; Godon, P. (2012), "White dwarfs in cataclysmic variable stars: accretion physics and evolution", Memorie della Societa Astronomica Italiana, 83: 539,
Bibcode:
2012MmSAI..83..539S.
Jiang, L. L.; et al. (January 2010), "The Photometry of Cataclysmic Variable V1159 Ori and BZ UMa", Acta Astronomica Sinica, 51 (1): 42–53,
Bibcode:
2010AcASn..51...42J.
Price, A.; et al. (May 2004), "Flickering and Periodic Activity in the 2004 Outburst of BZ UMa", Information Bulletin on Variable Stars, 5526 (1): 1,
Bibcode:
2004IBVS.5526....1P.
Kato, T. (September 1999), "CCD Photometry of the 1999 March Outburst of BZ UMa: Detection of Quasi-Periodic Oscillations", Information Bulletin on Variable Stars, 4768 (1): 1,
Bibcode:
1999IBVS.4768....1K.
Jurcevic, J. S.; et al. (May 1994), "Spectroscopy and Photometry of the Dwarf Nova BZ UMa and the CV Line-Width/K, Mass-Ratio Relation", Publications of the Astronomical Society of the Pacific, 106: 481,
Bibcode:
1994PASP..106..481J,
doi:10.1086/133403,
S2CID120863048.
Ringwald, F. A.; Thorstensen, J. R. (September 1990), "Quasi-Periodic Variation in the Radial Velocity Curve of the Dwarf Nova BZ UMa", Bulletin of the American Astronomical Society, 22: 1291,
Bibcode:
1990BAAS...22.1291R.