Results 11 to 20 of about 86,009 (222)
The outbursts of dwarf novae [PDF]
Monthly Notices of the Royal Astronomical Society, 2000 10 pages, 12 figures.
Truss, MR +3 more
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On the nature of superoutbursts in dwarf novae [PDF]
Monthly Notices of the Royal Astronomical Society, 2001 Typo corrected in caption to figure 2. LaTeX, 5 pages, 8 figures (1 colour).
Truss, M. R., Murray, J. R., Wynn, G. A.
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When does an old nova become a dwarf nova? Kinematics and age of the nova shell of the dwarf nova AT Cancri [PDF]
Monthly Notices of the Royal Astronomical Society, 2016 8 pages, 8 ...
Shara, Michael M. +4 more
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The Dwarf Novae during Quiescence [PDF]
The Astrophysical Journal, 2006 36 pages, 3 tables, 8 figures, final accepted version of ...
Sion, Edward, Urban, Joel
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The Temperatures of White Dwarfs in Dwarf Novae [PDF]
International Astronomical Union Colloquium, 1996 AbstractWe attempt to measure the temperature of all the quiescent dwarf novae that have been observed with IUE, by fitting the observed flux distribution of white dwarfs (WDs) with known temperatures. This approach gives results similar to those using much more sophisticated modelling, but allows us to investigate the relationship with system ...
B. J. M. Hassall, C. La Dous
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A DWARF NOVA IN THE GLOBULAR CLUSTER M13 [PDF]
The Astrophysical Journal, 2011 Accepted for publication in ApJ, 12 pages, 12 figures, 5 tables (v2 contains corrections of the proofs)
Servillat, M. +6 more
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International Astronomical Union Colloquium, 1995 AbstractThis report provides a summary of flares observed visually in the dwarf novae V442 Cen, OY Car, TU Men and Z Cha. The flares precede an outburst by an average of around ten days.
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The orbital and superhump periods of the dwarf nova HS 0417+7445 in Camelopardalis [PDF]
, 2011 We present the 2005-2010 outburst history of the SU UMa-type dwarf HS 0417+7445, along with a detailed analysis of extensive time-series photometry obtained in March 2008 during the second ecorded superoutburst of the system.
P. Dubovský +11 more
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X-ray variations in the inner accretion flow of dwarf novae
, 2021 Aims. We study the inner disk structure of dwarf novae (DNe; i.e., nonmagnetic cataclysmic variables)
BALMAN, Şölen, Revnivtsev, M.
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Observations of Eclipsing Dwarf Novae [PDF]
International Astronomical Union Colloquium, 1987 AbstractHigh Speed Photometry of four eclipsing dwarf novae, Z Cha, OY Car, HT Cas and IP Peg, is used to determine the orbital parameters and the masses of the two stars in each system. The mass ratio, q, and inclination, i, are found by constraining theoretical stream trajectories (Lubow and Shu 1975) to pass through the observed light centre of the ...
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