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Far Ultraviolet Spectroscopic Explorer Observations of the Blue Compact Dwarf Galaxy Markarian 59
New Far Ultraviolet Spectroscopic Explorer (FUSE) far-UV spectroscopy of the nearby metal-deficient (Zsolar/8) cometary blue compact dwarf (BCD) galaxy Markarian (Mrk) 59 is discussed. The data are used to investigate element abundances in its interstellar medium. The H I absorption lines are charac...
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Published in: | The Astrophysical journal 2002-02, Vol.565 (2), p.941-951 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | New Far Ultraviolet Spectroscopic Explorer (FUSE) far-UV spectroscopy of the nearby metal-deficient (Zsolar/8) cometary blue compact dwarf (BCD) galaxy Markarian (Mrk) 59 is discussed. The data are used to investigate element abundances in its interstellar medium. The H I absorption lines are characterized by narrow cores that are interstellar in origin and by broad wings that are stellar in origin. The mean interstellar H I column density is ~7Ă—1020 cm-2 in Mrk 59. No H2 lines are seen and N(H2) is |
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ISSN: | 0004-637X 1538-4357 |
DOI: | 10.1086/324684 |