Results 11 to 20 of about 82,748 (221)
Study of Photometric Variability of Selected SU UMa Dwarf Novae [PDF]
Acta Polytechnica CTU Proceedings, 2015 In this work we present time-resolved photometry of several poorly-studied dwarf novae during recent superoutbursts. Observations were made with a CCD, mounted on 50- and 60-cm telescopes of the Sternberg Astronomical Institute in Crimea in April - May ...
I. Voloshina, V. Metlov
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Inner Disk Structure of Dwarf Novae in the Light of X-Ray Observations [PDF]
Acta Polytechnica CTU Proceedings, 2015 Diversity of the X-ray observations of dwarf nova are still not fully understood. I review the X-ray spectral characteristics of dwarf novae during the quiescence in general explained by cooling flow models and the outburst spectra that show hard X-ray ...
S. Balman
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Investigation of Superhumps in SU UMa-type Dwarf Novae Based on the Observations of TESS [PDF]
The Astrophysical Journal, 2023 We report a superhumps analysis of seven SU UMa-type dwarf novae based on observations made by the Transiting Exoplanet Survey Satellite (TESS). Superhumps are seen during the superoutbursts of SU UMa-type dwarf novae. The monthlong data sets of TESS are
Wei Liu, Shengbang Qian
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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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Symbiotic Star T CrB as an Extreme SU UMa–type Dwarf Nova
The Astrophysical Journal Letters, 2023 T CrB is a symbiotic recurrent nova that exhibits quiescent and active phases between its classical nova eruptions. The statistical properties of these active phases have been poorly studied thus far. Because of that their nature remained unknown.
Krystian Iłkiewicz +2 more
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Search for sub-TeV Neutrino Emission from Novae with IceCube-DeepCore
The Astrophysical Journal, 2023 The understanding of novae, the thermonuclear eruptions on the surfaces of white dwarf stars in binaries, has recently undergone a major paradigm shift. Though the bolometric luminosity of novae was long thought to arise directly from photons supplied by
R. Abbasi +387 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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