Issue |
A&A
Volume 387, Number 1, May III 2002
|
|
---|---|---|
Page(s) | L10 - L12 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361:20020430 | |
Published online | 15 May 2002 |
Letter to the Editor
Probing the intracluster star-light with Chandra
1
Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, 85748 Garching, Germany
2
Smithsonian Astrophysical Observatory, 60 Garden st., MS 3, Cambridge, MA 02138, USA
3
Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, Hawaii 96822, USA
Corresponding author: A. Finoguenov, alexis@xray.mpe.mpg.de
Received:
5
October
2001
Accepted:
20
March
2002
We propose a method to test for the presence of intracluster star-light using X-ray binaries as a trace population. We discuss a particular application of this method to observations of the Virgo cluster.
Key words: stars: binaries: close / X-rays: stars / cosmology: observations
© ESO, 2002
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.