2800 MgII Doublet as an Indicator of Circumstellar Clouds |
| |
Authors: | GA Gurzadyan |
| |
Institution: | (1) Garny Space Astronomy Institute, Armenia |
| |
Abstract: | It is shown that the profiles and strengths of ultraviolet MgII doublet, k and h MgII lines, may be essentially different
in the spectra of two stars of one and the same spectral and luminosity class. This fact may be explained by the presence
of circumstellar clouds around the stars, particularly of B–A types. We demonstrate the possibility of the utilization of
2800 MgII doublet as an indicator of circumstellar clouds. The problem of three-scale spectral classification of stars is
raised.
This revised version was published online in July 2006 with corrections to the Cover Date. |
| |
Keywords: | |
本文献已被 SpringerLink 等数据库收录! |
|