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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Bibliographic Details
Main Authors: Schulz, Norbert S., Allen, Glenn E., Bautz, Mark W., Canizares, Claude R., Davis, John E., Dewey, Dan, Huenemoerder, David P., Heilmann, Ralf K., Houck, John C., Marshall, Herman Lee, Nowak, Michael A., Schattenburg, Mark
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:en_US
Published: National Academy of Sciences 2013
Online Access:http://hdl.handle.net/1721.1/77613
https://orcid.org/0000-0001-6932-2612
https://orcid.org/0000-0002-1379-4482
https://orcid.org/0000-0002-5769-8441

Internet

http://hdl.handle.net/1721.1/77613
https://orcid.org/0000-0001-6932-2612
https://orcid.org/0000-0002-1379-4482
https://orcid.org/0000-0002-5769-8441

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