Orbital and stochastic far-ultraviolet variability in the nova-like system V3885 Sgr-Reference-Cited by-同舟云学术

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Orbital and stochastic far-ultraviolet variability in the nova-like system V3885 Sgr

Published:2011-11-18 Issue:4 Volume:419 Page:3537-3546
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Prinja R. K.,Long K. S.,Richards M. T.,Witherick D. K.,Peck L. W.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference29 articles.

1. Hubble Space Telescope and R-Band Eclipse Maps of the UX Ursae Majoris Accretion Disk

2. High-velocity winds from a dwarf nova during outburst

3. Inclination and orbital-phase-dependent resonance line-profile calculations applied to cataclysmic variable winds

4. Absorption Line Profile Variations among the O Stars. I. The Incidence of Variability

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1. IMAGES OF GRAVITATIONAL AND MAGNETIC PHENOMENA DERIVED FROM TWO-DIMENSIONAL BACK-PROJECTION DOPPLER TOMOGRAPHY OF INTERACTING BINARY STARS;The Astrophysical Journal;2014-10-28

2. Explorations into 3D Doppler Tomography of Interacting Binaries;Proceedings of the International Astronomical Union;2012-08

3. Tomography of Interacting Binary Systems: Algols to Gamma-Ray Binaries;Proceedings of the International Astronomical Union;2011-07

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