Issue |
EAS Publications Series
Volume 63, 2013
New Advances in Stellar Physics: From Microscopic to Macroscopic Processes
|
|
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Page(s) | 411 - 413 | |
Section | Posters | |
DOI | https://doi.org/10.1051/eas/1363047 | |
Published online | 19 December 2013 |
New Advances in Stellar Physics: From Microscopic to Macroscopic Processes
G. Alecian, Y. Lebreton, O. Richard and G. Vauclair (eds)
EAS Publications Series, 63 (2013) 411–413
G. Alecian, Y. Lebreton, O. Richard and G. Vauclair (eds)
EAS Publications Series, 63 (2013) 411–413
Physical properties of HgMn stars on the basis of the available data
1 LUTH, Observatoire de paris, 5 place Jules Janssen, 92190 Meudon, France
2 Byurakan Astrophysical Observatory, Aragatsotn Province, Byurakan 0213, Armenia
a e-mail: satenik.ghazaryan@obspm.fr
A large database of HgMn stars is compiled, which contains the results of new measurements of their spectroscopic parameters combined with the data available in the literature. This database gives us an idea about the evolutionary changes of the HgMn stars.
© EAS, EDP Sciences, 2013