Results 1 to 10 of about 10,397 (194)
Spectroscopy of Nine Cataclysmic Variable Stars [PDF]
We present optical spectroscopy of nine cataclysmic binary stars, mostly dwarf novae, obtained primarily to determine orbital periods Porb. The stars and their periods are LX And, 0.1509743(5) d; CZ Aql, 0.2005(6) d; LU Cam, 0.1499686(4) d; GZ Cnc, 0 ...
Ann B. Kapusta +15 more
core +2 more sources
ABOUT THREE CATACLYSMIC VARIABLE STARS
In order to detect the new outbursts of the three cataclysmic variable TV Crv, NSV 1775, NSV 895, their positions was scanned on the plates of the Odessa collection of the sky service obtained for the period 1958 - 1988. The new outbursts were detected
A. V. Klabukova
doaj +2 more sources
Exploring the SDSS Dataset with Linked Scatter Plots: I. EMP, CEMP, and CV Stars. [PDF]
We present the results of a search for extremely metal-poor (EMP), carbon-enhanced metal-poor (CEMP), and cataclysmic variable (CV) stars using a new exploration tool based on linked scatter plots (LSPs).
Carbon DF, Henze C, Nelson BC.
europepmc +4 more sources
Parallax and Distance Estimates for Twelve Cataclysmic Variable Stars [PDF]
We report parallax and distance estimates for twelve more cataclysmic binaries and related objects observed with the 2.4m Hiltner telescope at MDM Observatory. The final parallax accuracy is typically about 1 mas.
Araujo-Betancor +37 more
core +5 more sources
The absence of jets in cataclysmic variable stars [PDF]
We show that the recently developed thermal model which successfully describes how jets are launched by young stellar objects, when applied to system containing disk-accreting white dwarfs naturally explain the otherwise surprising absence of jets in ...
Becker +41 more
core +5 more sources
An X-Ray-dim “Isolated” Neutron Star in a Binary?
We report the discovery of a dark companion to 2MASS J15274848+3536572 with an orbital period of 6.14 hr. Combining the radial velocity from LAMOST observations and modeling of the multiband light curve, one obtains a mass function of ≃0.131 M _⊙ , an ...
Jie Lin +15 more
doaj +1 more source
VY Sculptoris stars as magnetic cataclysmic variables [PDF]
AbstractWe show that VY Scl stars must be magnetized in order to account for the absence of outbursts during their low and intermediate states. Absence of outbursts during low states requires only rather low magnetic moments but in systems in which the drops and rises of luminosity are slower than it takes for the accretion disc to adjust viscously to ...
Hameury, J. -M., Lasota, J. -P.
openaire +3 more sources
Accretion in Cataclysmic Variable Stars [PDF]
We consider accretion onto the white dwarfs in cataclysmic variables in relation to nova eruptions, dwarf nova outbursts, hibernation and non-radial oscillations.
Warner, Brian, Woudt, Patrick A.
openaire +2 more sources
The spatial distribution, Galactic model parameters, and luminosity function of cataclysmic variables (CVs) are established using reestimated trigonometric parallaxes from Gaia DR3.
Remziye Canbay +3 more
doaj +1 more source
Cataclysmic Variable Stars [PDF]
AbstractThe properties of cataclysmic variable outbursts are reviewed, and interpreted in terms of dynamical instabilities by the red component, and subsequent evolution of the white dwarf accretion disc subject to a mass transfer burst in the transfer stream.
openaire +1 more source

