Award Date
1-1-2003
Degree Type
Thesis
Degree Name
Master of Science (MS)
Department
Physics
First Committee Member
Diane Pyper-Smith
Number of Pages
58
Abstract
Previous low-resolution spectroscopy has been used to find stars with highly active chromospheres within 50 pc of the Sun for the Northern hemisphere. We have analyzed thirteen such stars, using high-resolution spectroscopy, to determine Lithium abundances and metallicities. Although two of these stars may be close binaries, it is likely that eleven are single stars or wide binaries, of which four seem to be Pleiades age and two others appear Hyades age. It is usually expected that young stars are to be found in clusters, such as the Pleiades, in which there are many highly active young stars in close proximity to each other. However, we identify several apparently young single nearby field stars.
Keywords
Active; High; Resolution; Solar; Spectroscopy; Stars; Type
Controlled Subject
Astronomy
File Format
File Size
1884.16 KB
Degree Grantor
University of Nevada, Las Vegas
Language
English
Permissions
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Repository Citation
Drager, Nora Rae, "High-resolution spectroscopy of very active solar-type stars" (2003). UNLV Retrospective Theses & Dissertations. 1547.
http://dx.doi.org/10.25669/jljy-x6il
Rights
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