UV Line Emissions of W UMa Stars
We reinvestigate UV line emissions of 44i Boo, W UMa, AW UMa and VW Cep, which are indicaters of chromospheric activity of these stars. C I, C II, C IV, Si IV lines show significant variation in orbital phase. Among those lines, the Line of C IV showed the strongest line flux. while other Si IV and...
| Main Authors: | , , |
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| Format: | Article |
| Sprog: | English |
| Udgivet: |
The Korean Space Science Society
2000-06-01
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| Serier: | Journal of Astronomy and Space Sciences |
| Fag: | |
| Online adgang: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2000/v17n1/OJOOBS_2000_v17n1_39.pdf |