UV Energy Distribution of AZ Cassiopeiae
The IUE low dispersion spectra of AZ Cas have been analyzed for line identifications and energy distribution in ultraviolet region. Highly ionized atoms, Si IV and C IV are identified. We could infer a temperature range of the B star between 15,000K and 20,000K. The energy density distribution shows...
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| Format: | Article |
| Language: | English |
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Korean Space Science Society (KSSS)
1994-06-01
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| Series: | Journal of Astronomy and Space Sciences |
| Online Access: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1994/v11n1/OJOOBS_1994_v11n1_31.pdf |