Related records
Services
BibSonomy
CiteUlike
Connotea
Del.icio.us
Digg
Facebook
Free access article
|
||||||||||||||||||
A&A 387, L10-L12 (2002)
DOI: 10.1051/0004-6361:20020430
Letter
Probing the intracluster star-light with Chandra
A. Finoguenov1, 2, R. P. Kudritzki3 and C. Jones21 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
(Received 5 October 2001 / Accepted 20 March 2002)
Abstract
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
Offprint request: A. Finoguenov, alexis@xray.mpe.mpg.de
SIMBAD Objects
© ESO 2002
| What is OpenURL? |
The OpenURL standard is a protocol for transmission of metadata describing the resource that you wish to access. An OpenURL link contains article metadata and directs it to the OpenURL server of your choice. The OpenURL server can provide access to the resource and also offer complementary services (specific search engine, export of references...). The OpenURL link can be generated by different means.
- If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
- You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
- You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.