Findings from a Rochester Institute of Technology study provide further evidence that the outskirts of spiral galaxies host massive black holes. These overlooked regions are new places to observe gravitational waves created when the massive bodies collide, the authors report.
The study winds back time on massive black holes by analyzing their visible precursors—supernovae with collapsing cores. The slow decay of these massive stars creates bright signatures in the electromagnetic spectrum before stellar evolution ends in black holes.
Using data from the Lick Observatory Supernova Search, a survey of nearby galaxies, the team compared the supernovae rate in outer spiral galaxies with that of known hosts—dwarf/satellite galaxies—and found comparable numbers for typical spiral outskirts and typical dwarf galaxies, roughly two core-collapse supernovae per millennium.
The study, “Supernova Rate beyond the Optical Radius,” will appear in an upcoming issue of Astrophysical Journal Letters.
Low levels of elements heavier than hydrogen and helium found in dwarf/satellite galaxies create favorable conditions for massive black holes to form and create binary pairs. A similar galactic environment in the outer disks of spiral galaxies also creates likely hunting grounds for massive black holes, said Sukanya Chakrabarti, lead author and assistant professor in the RIT School of Physics and Astronomy.
“If these core-collapse supernovae are the predecessors to the binary black holes detected by LIGO (Laser Interferometer Gravitational-wave Observatory), then what we’ve found is a reliable method of identifying the host galaxies of LIGO sources,” said Chakrabarti. “Because these black holes have an electromagnetic counterpart at an earlier stage in their life, we can pinpoint their location in the sky and watch for massive black holes.”
The study’s findings complement Chakrabarti’s 2017 study, which showed that the outer parts of spiral galaxies could contribute to LIGO detection rates. The regions form stars at a comparable rate to dwarf galaxies and are low in heavy element content, creating a conducive home for massive black holes. The current study isolates potential candidates within these favorable galactic environments.
“We see now that these are both important contributors,” Chakrabarti said. “The next step is to do deeper surveys to see if we can improve the rate.”
Co-author Brennan Dell, a recent graduate from RIT’s computer science program, analyzed the data with Chakrabarti during his undergraduate co-op.
“This work may help us determine which galaxies to be on the lookout for electromagnetic counterparts of massive black holes,” Dell said.
Reference: “The Supernova Rate beyond the Optical Radius” by Sukanya Chakrabarti, Brennan Dell, Or Graur, Alexei V. Filippenko, Benjamin T. Lewis and Christopher F. McKee, 3 August 2018, The Astrophysical Journal Letters.
NASA and National Science Foundation awards funded Chakrabarti’s study and contributions from co-authors Dell and Benjamin Lewis at RIT’s Center for Computational Relativity and Gravitation; additional co-authors include Or Graur from Harvard-Smithsonian Center for Astrophysics; Alexei Filippenko at University of California, Berkeley, who leads the Lick Observatory Supernova Search; and Christopher McKee at the University of California, Berkeley.