# A fundamental plane in X-ray binary activity of external galaxies

@article{Inoue2021AFP,
title={A fundamental plane in X-ray binary activity of external galaxies},
author={Yoshiyuki Inoue and Kiyoto Yabe and Yoshihiro Ueda},
journal={Publications of the Astronomical Society of Japan},
year={2021}
}
• Yoshiyuki Inoue
• Published 2021
• Physics
• Publications of the Astronomical Society of Japan
We construct a new catalog of extragalactic X-ray binaries (XRBs) by matching the latest Chandra source catalog with local galaxy catalogs. Our XRB catalog contains 4430 XRBs hosted by 237 galaxies within ∼130 Mpc. As XRBs dominate the X-ray activity in galaxies, the catalog enables us to study the correlations between the total X-ray luminosity of a galaxy LX,tot, star formation rate $\dot{\rho }_\star$, and stellar mass M⋆. As previously reported, LX,tot is correlated with $\dot{\rho }_… Expand #### Figures and Tables from this paper #### References SHOWING 1-10 OF 94 REFERENCES High Mass X-ray Binaries as a Star Formation Rate Indicator in Distant Galaxies • Physics • 2002 Based on CHANDRA observations of nearby starburst galaxies and RXTE/ASM, ASCA and MIR-KVANT/TTM studies of high mass X-ray binary (HMXB) populations in the Milky Way and Magellanic Clouds, we proposeExpand X-ray binaries as the origin of nebular He II emission in low-metallicity star-forming galaxies • Physics • Astronomy & Astrophysics • 2019 The origin of nebular He II emission, which is frequently observed in low-metallicity (O/H) star-forming galaxies, remains largely an unsolved question. Using the observed anticorrelation of theExpand X-ray emission from star-forming galaxies – I. High-mass X-ray binaries • Physics • 2011 Based on a homogeneous set of X-ray, infrared and ultraviolet observations from Chandra, Spitzer, GALEX and 2MASS archives, we study populations of high-mass X-ray binaries (HMXBs) in a sample of 29Expand The Evolution of Normal Galaxy X-ray Emission Through Cosmic History: Constraints from the 6 Ms Chandra Deep Field-South We present measurements of the evolution of normal-galaxy X-ray emission from$z \approx\$ 0-7 using local galaxies and galaxy samples in the 6 Ms Chandra Deep Field-South (CDF-S) survey. The majorityExpand
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• 2019
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