Extreme Long Period Eclipsing Binary Epsilon Aurigae
From the study of a spectroscopic plate of epsilon Aurigae, we can measure the radial velocity and the relative abundance for this eclipsing binary. Calculated radial velocity is -37 Km/s and the abundance of [Fe] is estimated as -1.5.
Bewaard in:
| Hoofdauteurs: | , , |
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| Formaat: | Artigo |
| Taal: | Inglês |
| Gepubliceerd in: |
The Korean Space Science Society
1990-06-01
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| Reeks: | Journal of Astronomy and Space Sciences |
| Online toegang: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1990/v7n1/OJOOBS_1990_v7n1_47.pdf |
| Tags: |
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