Results 121 to 130 of about 125,367 (265)
Dwarf Nova Oscillations: New Results
, 2001 New and archived observations of VW Hyi in outburst show the occasional presence of optical Dwarf Nova Oscillations (DNOs) over the range of 18 - 40 s. There is a rapid increase in period near the end of outburst, at the same time that the EUV falls almost to zero, which we attribute to propellering. The DNOs return to a shorter period after this phase,
Warner, Brian, Woudt, Patrick
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Increasing supercycle lengths of active SU UMa-type dwarf novae [PDF]
, 2013 M. Otulakowska-Hypka, A. Olech
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A review of the disc instability model for dwarf novae, soft X-ray transients and related objects [PDF]
, 2019 J. Hameury
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On the of classification of BL Her subtype of the Type II Cepheids
EPJ Web of Conferences, 2015 The initial reason for studying Type II Cepheids (CWB) was for period changes, binarity or any other signs of change other than the pulsation. The GCVS contained 71 objects of this kind in 2012 when the wok started, and that list is now extended to 100 ...
Jurkovic Monika I.
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Dwarf novae in the Hamburg quasar survey: rarer than expected [PDF]
, 2006 A. Aungwerojwit +14 more
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The EUVE Observations of Dwarf Novae [PDF]
International Astronomical Union Colloquium, 1996 In the standard theory of dwarf novae in outburst, the boundary layer region between the inner edge of the accretion disk and the white dwarf surface radiates primarily in the extreme ultraviolet. Using EUVE, observers have been able to obtain spectra with sufficient spectral resolution to characterize accurately the emission from several dwarf novae ...
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A Demarcation Criterion for Hydrogen Burning of Millinovae
The Astrophysical JournalMillinovae are a new class of transient supersoft X-ray sources with no clear signature of mass ejection. They show similar triangle shapes of V / I band light curves with 1000 times fainter peaks than typical classical novae. Maccarone et al.
Izumi Hachisu, Mariko Kato
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Odessa Astronomical Publications, 2010 We present a review of highlights of our photometric and photo-polarimetric monitoring and mathematical modeling of interacting binary stars of different types classical, asynchronous, intermedi ate polars with 25 timescales corresponding to differ ent ...
I. L. Andronov +25 more
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A Simple, Unifying Model of the Extreme Ultraviolet Spectra of Dwarf Novae in Outburst [PDF]
, 2004 Christopher W. Mauche
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