A detached stellar-mass black hole candidate in the globular cluster NGC 3201

17 Jan 2018  ·  Giesers Benjamin, Dreizler Stefan, Husser Tim-Oliver, Kamann Sebastian, Escude Guillem Anglada, Brinchmann Jarle, Carollo C. Marcella, Roth Martin M., Weilbacher Peter M., Wisotzki Lutz ·

As part of our massive spectroscopic survey of 25 Galactic globular clusters with MUSE, we performed multiple epoch observations of NGC 3201 with the aim of constraining the binary fraction. In this cluster, we found one curious star at the main-sequence turn-off with radial velocity variations of the order of 100 km/s, indicating the membership to a binary system with an unseen component since no other variations appear in the spectra... Using an adapted variant of the generalized Lomb-Scargle periodogram, we could calculate the orbital parameters and found the companion to be a detached stellar-mass black hole with a minimum mass of 4.36 $\pm$ 0.41 solar masses. The result is an important constraint for binary and black hole evolution models in globular clusters as well as in the context of gravitational wave sources. read more

PDF Abstract
No code implementations yet. Submit your code now


Solar and Stellar Astrophysics Astrophysics of Galaxies