Ojha, D. K. ; Joshi, S. C. (1991) On the shell star pleione (BU Tauri) Journal of Astrophysics and Astronomy, 12 (3). pp. 213-223. ISSN 0250-6335
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Official URL: http://www-old.ias.ac.in/j_archive/jaa/12/vol12con...
Related URL: http://dx.doi.org/10.1007/BF02702879
Abstract
BU Tauri (Pleione) an interesting star in the Pleiades cluster, has been observed spectrophotometrically. The energy distribution curves of the star have been discussed vis a vis model atmospheres for normal stars in the appropriate range of temperature and effective gravity. The changes in the energy distribution curve noticed during our observations and previous observations taken from the literature have been pointed out. On the basis of the measured Há emission equivalent width, a rough estimate of the dimensions of the extended envelope of the star has been made.
Item Type: | Article |
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Source: | Copyright of this article belongs to Indian Academy of Sciences. |
Keywords: | Be Star; Energy Distribution |
ID Code: | 105754 |
Deposited On: | 26 Apr 2017 16:50 |
Last Modified: | 26 Apr 2017 16:50 |
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