Astro2020 Science White Paper: Populations of Black Holes in Binaries

Thomas J. Maccarone; Laura Chomiuk; James Miller-Jones; Eric Bellm; Katelyn Breivik; Chris L. Fryer; Vicky Kalogera; Shane Larson; Jerome Orosz; James F. Steiner; Jay Strader; John A. Tomsick

arXiv · 1904.11842

Astro2020 Science White Paper: Populations of Black Holes in Binaries

Thomas J. Maccarone·Laura Chomiuk·James Miller-Jones·Eric Bellm·Katelyn Breivik·Chris L. Fryer·Vicky Kalogera·Shane Larson·Jerome Orosz·James F. Steiner·Jay Strader·John A. Tomsick

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Abstract

Black holes in binary star systems are vital for understanding the process of pr oducing gravitational wave sources, understanding how supernovae work, and for p roviding fossil evidence for the high mass stars from earlier in the Universe. At the present time, sample sizes of these objects, and especially of black hole s in binaries, are quite limited. Furthermore, more precise measurements of the binary parameters are needed, as well. With improvements primarily in X-ray an d radio astronomy capabilities, it should be possible to build much larger sampl es of much better measured black hole binaries.

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Thomas J. Maccarone, Laura Chomiuk, James Miller-Jones, Eric Bellm, Katelyn Breivik, Chris L. Fryer, Vicky Kalogera, Shane Larson, Jerome Orosz, James F. Steiner, Jay Strader, John A. Tomsick. 2019-04-26. Astro2020 Science White Paper: Populations of Black Holes in Binaries. https://arxiv.org/abs/1904.11842

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