High-mass X-ray binaries in a cosmological context

María Celeste Artale, Leonardo J. Pellizza, Patricia B. Tissera, I. Felix Mirabel

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

Recent observational and theoretical results suggest that the production rates and luminosities of high-mass X-ray binaries depend on metallicity. To test this prediction, we combine HMXB population synthesis results with numerical simulations of galaxy formation to produce synthetic populations of HMXBs in star-forming galaxies, and compare the model predictions to observations of HMXB populations in nearby and high-redshift galaxies. Our models show a fair agreement with observations only when the HMXB production and luminosities are assumed to depend strongly on metallicity.

Original languageEnglish
Title of host publicationFeeding Compact Objects
Subtitle of host publicationAccretion on All Scales
EditorsChengmin Zhang, Tomaso Belloni, Mariano Mendez, Shuangnan Zhang
Pages183-184
Number of pages2
EditionS290
DOIs
Publication statusPublished - Aug 2012

Publication series

NameProceedings of the International Astronomical Union
NumberS290
Volume8
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

Keywords

  • X-ray: binaries
  • evolution
  • galaxies - stars: evolution - galaxies: abundances

ASJC Scopus subject areas

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'High-mass X-ray binaries in a cosmological context'. Together they form a unique fingerprint.

Cite this