Krishna Swamy, K. S. (1970) Analysis of the hyades giant stars ε and γ Tau Astrophysics and Space Science, 8 (1). pp. 86-89. ISSN 0004-640X
|
PDF
- Publisher Version
204kB |
Official URL: http://www.springerlink.com/content/g33170r6242245...
Related URL: http://dx.doi.org/10.1007/BF00651658
Abstract
Two hyades giant stars, ε and γ Tau, have been studied from an analysis of strong line profiles. We get for ε Tau,Te =4750K and logg=2.7, and for γ Tau,Te =4700K and logg=2.8. Hydrogen-to-metal ratio for the two stars is nearly the same as that of solar value.
Item Type: | Article |
---|---|
Source: | Copyright of this article belongs to Springer-Verlag. |
ID Code: | 18251 |
Deposited On: | 17 Nov 2010 12:54 |
Last Modified: | 17 May 2016 02:59 |
Repository Staff Only: item control page