Results 31 to 40 of about 627 (186)

The Galactic kinematics of cataclysmic variables [PDF]

open access: yesAstrophysics and Space Science, 2015
Kinematical properties of CVs were investigated according to population types and orbital periods, using the space velocities computed from recently updated systemic velocities, proper motions and parallaxes. Reliability of collected space velocity data are refined by removing 34 systems with largest space velocity errors.
Ak, T.   +7 more
openaire   +5 more sources

The pre-cataclysmic variable, LTT 560 [PDF]

open access: yesAstronomy & Astrophysics, 2007
System parameters of the object LTT560 are determined in order to clarify its nature and evolutionary status. We apply time-series photometry to reveal orbital modulations of the light curve, time-series spectroscopy to measure radial velocities of features from both the primary and the secondary star, and flux-calibrated spectroscopy to derive ...
Tappert, Claus   +5 more
openaire   +4 more sources

Rapid oscillations in cataclysmic variables [PDF]

open access: yesAstrophysics and Space Science, 1986
I give an overview of the rich phenomenology of dwarf nova oscillations (DNOs) and Quasi-periodic Oscillations (QPOs) observed in cataclysmic variable stars (CVs). The favoured interpretation of these rapid brightness modulations (3 - >1000 s time scales) is that they are magnetic in nature - magnetically channelled accretion from the inner ...
openaire   +3 more sources

X-rays from cataclysmic variables [PDF]

open access: yes, 2006
40 pages, 10 figures; minor updates to text. To appear in Compact Stellar X-Ray Sources, eds. W.H.G. Lewin and M.
Kuulkers, E.   +3 more
openaire   +2 more sources

MAGNETIC CATACLYSMIC VARIABLES: 25 YEARS OF EXCITING PERFOMANCE

open access: yesOdessa Astronomical Publications, 2017
Exactly 25 years ago, Santiago Tapia has detected circular and linear polarization of AM Her varying with the same period as the photometric and spectral characteristics. This had lead to a discovery of unprecedentedly exotic binary systems, in which the
I. L Andronov
doaj   +1 more source

Ultraviolet observations of cataclysmic variables [PDF]

open access: yesAdvances in Space Research, 1987
AbstractThe preliminary results of the analysis of more than 1000 spectra of cataclysmic variables in the archive of the International Ultraviolet Explorer were presented at the meeting. To characterize the slope of the spectra I use F = log(f1460Å/f2880Å). For most spectra F lies between 0.2 and 0.7.
openaire   +1 more source

THE WINDS OF CATACLYSMIC VARIABLES [PDF]

open access: yes, 2018
19 pages, TeX format, 6 Postscript figures, uses mauche.mac and cwhstuff.tex. To appear in Cosmic Winds and the Heliosphere, ed. J. R. Jokipii, C. P. Sonett, & M. S. Giampapa (Tucson: Univ. of Arizona Press)
Mauche, C. W., Raymond, J. C.
openaire   +2 more sources

Brown dwarfs in retrogradely precessing cataclysmic variables?

open access: yesEPJ Web of Conferences, 2011
We compare Smoothed Particle Hydrodynamic simulations of retrogradely precessing accretion disks that have a white dwarf primary and a main sequence secondary with observational data and with theory on retrograde precession via tidal torques like those ...
Martin E.L.   +2 more
doaj   +1 more source

The ethics of responding to democratic backsliding abroad

open access: yesAmerican Journal of Political Science, EarlyView.
Abstract The past decade has seen a marked shift as many previously liberal democratic states have backslidden, taking authoritarian turns. How should liberal actors respond to democratic backsliding by others? Although it might seem that it is vital for liberal actors to react robustly to avoid complicity or to maintain their liberal integrity, this ...
James Pattison
wiley   +1 more source

Cataclysmic variables: structure and evolution [PDF]

open access: yesInternational Astronomical Union Colloquium, 1994
AbstractI discuss the structure and evolution of cataclysmic variables, with a particular emphasis on the influence of the physics used in calculating the internal structure of the secondary. The available observational data is very rich, and can, in principle, be used to constrain the stellar physics.
openaire   +1 more source

Home - About - Disclaimer - Privacy