2018/06/07 by Todd A. Thompson, Christopher S. Kochanek, Krzysztof Z. Stanek +14 · 1 voice
Physics and Astronomy · #astro-ph.HE #astro-ph.SR
paper · pdf · doi:10.1126/science.aau4005
Submitted. 57 pages, 12 figures; main text and supplementary material updated
arxiv published 2018/06/07 · arxiv created 2019/04/05 · arxiv updated 2019/11/20
We report the discovery of the first likely black hole in a non-interacting binary system with a field red giant. By combining radial velocity measurements from the Apache Point Observatory Galactic Evolution Experiment (APOGEE) with photometric variability data from the All-Sky Automated Survey for Supernovae (ASAS-SN), we identified the bright rapidly-rotating giant 2MASS J05215658+4359220 as a binary system with a massive unseen companion. Subsequent radial velocity measurements reveal a system with an orbital period of 83 days and near-zero eccentricity. The photometric variability period of the giant is consistent with the orbital period, indicative of star spots and tidal synchronization. Constraints on the giant's mass and radius from its luminosity, surface gravity, and temperature imply an unseen companion with mass of 3.3+2.8-0.7 M_\odot, indicating a low-mass black hole or an exceedingly massive neutron star. Measurement of the astrometric binary motion by \it Gaia will further characterize the system. This discovery demonstrates the potential of massive spectroscopic surveys like APOGEE and all-sky, high-cadence photometric surveys like ASAS-SN to revolutionize our understanding of the compact object mass function, and to test theories of binary star evolution and the supernova mechanism.