The Shape of Long Outbursts in U Gem Type Dwarf Novae from AAVSO Data [PDF]
We search the American Association of Variable Star Observers (AAVSO) archives of the two best studied dwarf novae in an attempt to find light curves for long outbursts that are extremely well-characterized. The systems are U Gem and SS Cyg.
Cannizzo, John K.
core +5 more sources
Characterization of Dwarf Novae Using SDSS Colors [PDF]
We have developed a method for estimating the orbital periods of dwarf novae from the Sloan Digital Sky Survey (SDSS) colors in quiescence using an artificial neural network.
Kato, Taichi +2 more
core +4 more sources
For Galactic novae, I calculate and collect a comprehensive catalog of 208 measures of white dwarf (WD) masses ( M _WD ) and 232 measures of average V magnitudes in quiescence ( V _q ). These are collected into a comprehensive catalog of most fundamental
Bradley E. Schaefer
doaj +2 more sources
Dwarf Novae in the Shortest Orbital Period Regime: II. WZ Sge Stars as the Missing Population near the Period Minimum [PDF]
WZ Sge-type dwarf novae are characterized by long recurrence times of outbursts (~10 yr) and short orbital periods (
Kato, T. +3 more
core +3 more sources
Classical Novae Masquerading as Dwarf Novae? Outburst Properties of Cataclysmic Variables with ASAS-SN [PDF]
The unprecedented sky coverage and observing cadence of the All-Sky Automated Survey for SuperNovae (ASAS-SN) has resulted in the discovery and continued monitoring of a large sample of Galactic transients.
A. Kawash +14 more
semanticscholar +1 more source
On the Limits of Alpine Plants: A Systematic Review of the Factors Behind Species' Elevational Range Limits. [PDF]
This systematic review of 107 studies on the factors behind the elevational range limits of alpine vascular plants shows a persistent emphasis on upper limits and abiotic factors, especially temperature, while work at lower limits is more evenly distributed across water availability, plant–plant interactions, and selection/local adaptation.
Weides SE +7 more
europepmc +2 more sources
The outbursts of dwarf novae [PDF]
10 pages, 12 figures.
Truss, MR +3 more
openaire +3 more sources
Thermal-viscous instability in tilted accretion disks: A possible application to IW Andromeda-type dwarf novae [PDF]
IW And stars are a subgroup of dwarf novae characterized by repetition of the intermediate brightness state with oscillatory variations terminated by brightening.
M. Kimura +3 more
semanticscholar +1 more source
Turbulent and wind-driven accretion in dwarf novae threaded by a large-scale magnetic field [PDF]
Dwarf novae (DNe) are accreting white dwarfs that show eruptions caused by a thermal-viscous instability in the accretion disk. The outburst timescales constrain α, the ratio of the viscous stress to the thermal pressure, which phenomenologically ...
N. Scepi, G. Lesur, G. Dubus, M. Flock
semanticscholar +1 more source
On the nature of superoutbursts in dwarf novae [PDF]
Typo corrected in caption to figure 2. LaTeX, 5 pages, 8 figures (1 colour).
Truss, M. R., Murray, J. R., Wynn, G. A.
openaire +4 more sources

