Structure and Evolution of Pre-Main Sequence Stars

Structure and Evolution of Pre-Main Sequence Stars

Low-mass pre-main sequence (PMS) stars are strong and variable X-ray emitters, as has been well established by EINSTEIN and ROSAT observatories. It was originally believed that this emission was of thermal nature and primarily originated from coronal activity (magnetically confined loops, in analogy...

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Main Authors: Schulz, Norbert S. (Contributor), Allen, Glenn E. (Contributor), Bautz, Mark W. (Contributor), Canizares, Claude R. (Contributor), Davis, John E. (Contributor), Dewey, Dan (Contributor), Huenemoerder, David P. (Contributor), Heilmann, Ralf K. (Contributor), Houck, John C. (Contributor), Marshall, Herman Lee (Contributor), Nowak, Michael A. (Contributor), Schattenburg, Mark (Contributor)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: National Academy of Sciences, 2013-03-11T15:04:24Z.
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