Results 111 to 120 of about 2,620,915 (156)
Nonmagnetic cataclysmic variables (CVs) show two distinct X-ray components: a hard, optically thin component and a soft, optically thick, blackbody-like component, both produced in the boundary layer between the accretion disk and the white dwarf (WD ...
Nazma Islam +3 more
doaj +1 more source
An Equipotential Disk Model with Irradiation for Nova-like Variables
The reflection effect is here incorporated within an earlier analytic binary system light- and velocity-curve model that includes a circumstellar equipotential disk.
R. E. Wilson, W. Van Hamme
doaj +1 more source
Balmer decrements as a new diagnostic for period-bounce cataclysmic variable stars
Context. Cataclysmic variable stars (CVs) evolve towards shorter orbital periods (Porb) until they reach a minimum Porb of ∼80 min. Beyond this point, the donor star becomes out of thermal equilibrium or increasingly degenerate, causing the system to ...
Hernández-Díaz Santiago +2 more
doaj +1 more source
Sonification of Kepler Field SU UMa Cataclysmic Variable Stars V344 Lyr and V1504 Cyg [PDF]
Sonification is the conversion of quantitative data into sound. In this work we explain the methods used in the sonification of light curves provided by the Kepler instrument from Q2 through Q6 for the cataclysmic variable systems V344 Lyr and V1504 Cyg .
Cannizzo, John K. +5 more
core
A program of long-term ground-based photometric monitoring of 134 old novae and novalike cataclysmic variables (CVs) has been concluded. In this paper, we display, analyze, and discuss the light curves of 33 of these targets, which have shown “stunted ...
R. K. Honeycutt +2 more
doaj +1 more source
On the Masses of Cataclysmic Variable Stars [PDF]
openaire +1 more source
Detection of Transitions between Dwarf Nova Outbursts, Standstills, and IW And–type Cycles
IW And–type objects represent a rare and intriguing subclass of cataclysmic variables that challenge the classical disk instability model. Due to their long timescales, often lasting several months, observed samples are scarce, leaving the physics of ...
Qi-Bin Sun +8 more
doaj +1 more source
Investigation of the new cataclysmic variable 1RXS J180834.7+101041
We present the results of our photometric and spectroscopic studies of the new eclipsing cataclysmic variable star 1RXS J180834. 7+101041. Its spectrum exhibits double-peaked hydrogen and helium emission lines.
Suleimanov V. +4 more
core
Modeling Varying Mass Transfer in Cataclysmic Variable Stars
Color poster with text, images, charts, and graphs.This research details the results of work done in Modules for Experiments in Stellar Astrophysics (MESA) on cataclysmic variables.
Mohamed, Mahdi
core
Erratum: The donor stars of cataclysmic variables [PDF]
openaire +1 more source

