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Using High-Mass X-ray binaries to probe massive binary evolution: The age distribution of High-Mass X-ray binaries in M33

Published online by Cambridge University Press:  30 December 2019

Kristen Garofali Open the ORCID record for Kristen Garofali [Opens in a new window]  and
Benjamin F. Williams
Kristen Garofali
Affiliation:
Department of Astronomy, University of WashingtonBox 351580, U.W., Seattle, WA, USA emails: [email protected], [email protected] Department of Physics, University of Arkansas, 825 West Dickson St, Fayetteville, AR, USA email: [email protected]
Benjamin F. Williams
Affiliation:
Department of Astronomy, University of WashingtonBox 351580, U.W., Seattle, WA, USA emails: [email protected], [email protected]
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Abstract

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High-mass X-ray binaries (HMXBs) provide an exciting window into the underlying processes of both binary as well as massive star evolution. Because HMXBs are systems containing a compact object accreting from a high-mass star at close orbital separations they are also likely progenitors of gamma-ray bursts and gravitational wave sources. We present classification and age measurements for HMXBs in M33 using a combination of deep Chandra X-ray imaging, and archival Hubble Space Telescope data. We constrain the ages of the HMXB candidates by fitting the color-magnitude diagrams of the surrounding stars, which yield the star formation histories of the surrounding region. Unlike the age distributions measured for HMXB populations in the Magellanic Clouds, the age distribution for the HMXB population in M33 contains a number of extremely young (<5 Myr) sources. We discuss these results the context of the effect of host galaxy properties on the observed HMXB population.

Keywords

X-rays: binariesLocal Groupstars: imaging
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S346: High-mass X-ray Binaries: Illuminating the Passage from Massive Binaries to Merging Compact Objects , August 2018 , pp. 322 - 331
Copyright
© International Astronomical Union 2019 

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