A Synthetic Spectrum and Light‐Curve Analysis of the Cataclysmic Variable IX Velorum-Reference-Cited by-同舟云学术

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A Synthetic Spectrum and Light‐Curve Analysis of the Cataclysmic Variable IX Velorum

Published:2007-06-20 Issue:2 Volume:662 Page:1204-1219
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Linnell Albert P.,Godon Patrick,Hubeny Ivan,Sion Edward M.,Szkody Paula

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference86 articles.

1. Allen, C. W. 1973, Astrophysical Quantities (3rd ed.; London: Athlone)

2. A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution

3. Magnetic Pressure Support and Accretion Disk Spectra

4. Bohnhardt, H., Dreschel, H., Rahe, J. & Wargau, W. 1982, IAU Circ. 3749

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1. Revisiting the accretion disc spectra of dwarf novae and nova-like variables: implications for the standard disc model;Monthly Notices of the Royal Astronomical Society;2024-06-07

2. Structure of the accretion flow of IX Velorum as revealed by high-resolution spectroscopy;Astronomy & Astrophysics;2023-10

3. An improved model for the spectra of discs of nova-like variables;Monthly Notices of the Royal Astronomical Society;2021-03-22

4. Structure of accretion flows in the nova-like cataclysmic variable RW Tri;Monthly Notices of the Royal Astronomical Society;2020-07-20

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