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A FIRST ESTIMATE OF THE X-RAY BINARY FREQUENCY AS A FUNCTION OF STAR CLUSTER MASS IN A SINGLE GALACTIC SYSTEM

Author
CLARK, D. M1 2 ; EIKENBERRY, S. S2 ; BRANDL, B. R3 ; WILSON, J. C4 ; CARSON, J. C5 ; HENDERSON, C. P6 ; HAYWARD, T. L7 ; BARRY, D. J4 ; PTAK, A. F8 ; COLBERT, E. J. M8
[1] Instituto de Astronomia, Universidad Nacional Autónoma de México, Apdo Postal 877, Ensenada, Baja Califomia, Mexico
[2] Department of Astronomy, University of Florida, Gainesville, FL 32611, United States
[3] Leiden University, P.O. Box 9513, 2300 RA Leiden, Netherlands
[4] Department of Astronomy, P.O Box 400325, University of Virginia, Charlottesville, VA 22904, United States
[5] Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
[6] Astronomy Department, Comell University, Ithaca, NY 14853, United States
[7] Gemini Observatory, AURA/Casilla 603, La Serena, Chile
[8] Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218, United States
Source

The Astrophysical journal. 2008, Vol 678, Num 2, pp 798-803, 6 p ; 1 ; ref : 1/4 p

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Author keyword
X-rays: binaries galaxies: star clusters galaxies: starburst
Keyword (fr)
Amas galaxies Amas stellaire Binaire RX Galaxies à flambée Masse stellaire Source RX binaire Source RX cosmique
Keyword (en)
Galaxy clusters Star clusters X-ray binary stars Starburst galaxies Stellar mass Binary X ray source Cosmic x-ray sources
Keyword (es)
Galaxias llamarada estelar Fuente RX binaria
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20317552

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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