Coronal and Transition Region Structure in the RS Canum Venaticorum Binaries V711 Tauri, AR Lacertae, and II Pegasi. I. Data Analysis and Emission Measure Distributions-Reference-Cited by-同舟云学术

Coronal and Transition Region Structure in the RS Canum Venaticorum Binaries V711 Tauri, AR Lacertae, and II Pegasi. I. Data Analysis and Emission Measure Distributions

Published:1998-04-20 Issue:2 Volume:497 Page:883-895
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Griffiths N. W.,Jordan C.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/497/i=2/a=883/pdf

Reference74 articles.

1. Binary phase correlated X-ray intensity variations and flaring activity in the RS CVn binary HR 1099

2. Abundances of the elements: Meteoritic and solar

3. Rate coefficients for the excitation of infrared and ultraviolet lines in C II, N III, and O IV

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