Results 91 to 100 of about 2,487,342 (212)
A New Window for Studying Intermediate Polars and Tilted Accretion Disk Precession
The Astrophysical JournalTV Col is a long-period eclipsing intermediate polar (IP) prototype star for the negative superhump (NSH) system. We investigate the eclipse minima, eclipse depth, and NSH amplitude based on TESS photometry.
Qi-Bin Sun +7 more
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Gas flow in cataclysmic variable stars
The Astrophysical Journal, 1975 A numerical hydrodynamic scheme, applicable to gas flow in binary stars, is presented which incorporates the effects of pressure and gravitational forces, radiative cooling, and shock formation. The method is used to study gas flow originating from Roche lobe overflow through the inner Lagrangian point, L$sub 1$, in a binary star modeled to resemble ...
openaire +1 more source
The Astrophysical JournalCompact objects undergoing mass transfer exhibit significant (and double-peaked) H _α emission lines. Recently, new methods have been developed to identify black hole X-ray binaries and calculate their systematic parameters using H _α line parameters ...
Xinlin Zhao, Song Wang, Jifeng Liu
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EUVE J0854+390: a new Cataclysmic Variable [PDF]
, 2001 We report the identification of a new CV in the field of EUVE J0854+390. The optical spectra show Balmer, He I and He II lines strongly in emission and indicates the source is a CV, probably magnetic.Information Bulletin on Variable Stars 5032(1).
B. Roberts +3 more
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The Astrophysical Journal Supplement SeriesBased mainly on the months-long 2 minutes time-resolution light curves observed by the Transiting Exoplanet Survey Telescope (TESS) space mission of 48 eclipsing old novae and novalike variables (commonly referred to as NLs) selected from the Ritter ...
Albert Bruch
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Time-resolved spectroscopy of the AM Herculis-type binary systems QQ VUL and EF ERI
, 1998 Cataclysmic variable stars (CVs) are interacting binary systems. One of the stars (referred to as the primary) is a white dwarf, the other (referred to as the secondary) is usually a late main sequence star such as a red dwarf.
Blakelock, Carolyn J.
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Optical identification of IGR J18308-1232 as a cataclysmic variable [PDF]
, 2008 We report on a spectroscopic analysis of optical sources inside the error circle of the XMM-Newton slew source XMMLS1 J183049.6-123218 (see Ibarra et al., ATel #1527), associated with the unidentifiedINTEGRAL source IGR J18308-1232 (Bird et al.
VAHRAM CHAVUSHYAN
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Mapeamento espectral de discos de acréscimo em variáveis cataclísmicas [PDF]
, 2008 Tese (doutorado) - Universidade Federal de Santa Catarina, Centro de Ciências Físicas e Matemáticas. Programa de Pós-Graduação em Física.Esta tese de doutorado é a continuação da dissertação de mestrado defendida em 2004. Nosso projeto visa analisar, com
Saito, Roberto Kalbusch
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1RXS J173021.5-055933 : a cataclysmic variable with a fast-spinning magnetic white dwarf [PDF]
, 2008 Aims. We present the first X-ray observations with the XMM-Newton and INTEGRAL satellites of the recently discovered cataclysmic variable 1RXS J173021.5-055933, together with simultaneous UV and coordinated optical photometry aiming at characterising its
Matt, Giorgio +42 more
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Resolving the Periods of the Asynchronous Polar 1RXS J083842.1–282723
The Astrophysical Journal1RXS J083842.1−282723 is a nearly synchronous magnetic cataclysmic variable with a simple X-ray light curve. While its orbital period was fairly well established at P _orb = 98.4 minutes from optical spectroscopy, indirect estimates of P _spin / P _orb ...
J. P. Halpern
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