Issue |
A&A
Volume 499, Number 3, June I 2009
|
|
---|---|---|
Page(s) | 891 - 891 | |
Section | Stellar atmospheres | |
DOI | https://doi.org/10.1051/0004-6361/20077141e | |
Published online | 25 March 2009 |
The black hole binary nova Scorpii 1994 (GRO J1655-40): an improved chemical analysis*
1
Observatoire de Paris-Meudon, GEPI, 5 place Jules Janssen, 92195 Meudon Cedex, France e-mail: Jonay.Gonzalez-Hernandez@obspm.fr
2
CIFIST Marie Curie Excellence Team
3
Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain e-mail: [rrl;gil]@iac.es
4
Consejo Superior de Investigaciones Científicas, Spain
This article has no abstract.
Key words: black holes physics / stars: abundances / stars: individual: Scorpii 1994 (GRO J1655-40) / stars: supernovae: general / X-rays: binaries / errata, addenda
© ESO, 2009
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.