Peculiar early-type supergiants and LBVs: resemblance and difference
- UNCG Author/Contributor (non-UNCG co-authors, if there are any, appear on document)
- Anatoly S. Miroshnichenko, Professor (Creator)
- Institution
- The University of North Carolina at Greensboro (UNCG )
- Web Site: http://library.uncg.edu/
Abstract: Peculiar early-type supergiants (hereafter PETS) have been distinguished from normal ones because of stronger emission lines in their spectra. This is a result of different stellar wing kinematics: PETS have slower winds with low terminal velocities – nearly 10 times smaller than those of normal supergiants.
Peculiar early-type supergiants and LBVs: resemblance and difference
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Created on 1/1/1997
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Additional Information
- Publication
- Astronomical Society of the Pacific Conference Series 120, 202
- Language: English
- Date: 1997
- Keywords
- stars, peculiar early-type supergiants