Application of Realistic Model Atmospheres to Eclipse Maps of Accretion Disks: The Effective Temperature and Flare of the Disk in the Dwarf Nova Z Chamaeleontis-Reference-Cited by-同舟云学术

Application of Realistic Model Atmospheres to Eclipse Maps of Accretion Disks: The Effective Temperature and Flare of the Disk in the Dwarf Nova Z Chamaeleontis

Published:1999-04 Issue:2 Volume:514 Page:952-958
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Robinson Edward L.,Wood Janet H.,Wade Richard A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/514/i=2/a=952/pdf

Reference39 articles.

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

2. The southern dwarf nova, Z Chamaeleontis.

3. Bateson, F. M. 1992, Circ. Royal Astron. Soc. New Zealand, M92/1-M92/7

4. High-speed photometry of Z Chamaeleontis covering the 1983 March normal outburst

5. Frank, J., King, A. R. & Raine, D. J. 1985, Accretion Power in Astrophysics (Cambridge: Cambridge Univ. Press)

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