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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.

Tallennettuna:
Bibliografiset tiedot
Päätekijät: Mun-Suk Chun, Jang-Hyeon Park, Jang-Hae Jeong
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: The Korean Space Science Society 1990-06-01
Sarja:Journal of Astronomy and Space Sciences
Linkit:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1990/v7n1/OJOOBS_1990_v7n1_47.pdf
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