Probable Detection of a Bright Infrared Coronal Emission Line of Siixnear 3.93 Microns-Reference-Cited by-同舟云学术

Probable Detection of a Bright Infrared Coronal Emission Line of Siixnear 3.93 Microns

Published:1999-08-10 Issue:1 Volume:521 Page:478-482
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Kuhn J. R.,MacQueen R. M.,Streete J.,Tansey G.,Mann I.,Hillebrand P.,Coulter R.,Lin H.,Edmunds D.,Judge P.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/521/i=1/a=478/pdf

Reference19 articles.

1. Bastian, T. 1995, in Infrared Tools for Solar Astrophysics: What’s Next? ed. J. R. Kuhn & M. J. Penn (Singapore: World Scientific), 115

2. Chang, E. S. & Deming, D. 1995, in Infrared Tools for Solar Astrophysics: What’s Next? ed. J. R. Kuhn & M. J. Penn (Singapore: World Scientific), 47

3. Coronal magnetic fields

4. Infrared coronal emission lines and the possibility of their laser emission in Seyfert nuclei

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