Neutron stars and black holes are the remnants of lifeless stars. They sometimes type as a part of a supernova explosion, the place the outer layers of an outdated star are violently forged off whereas the core of the star collapses to type the remnant. This violent origin can have important penalties for each the remnant and the encompassing surroundings.
One factor that may occur is that the remnant can get a “natal kick,” which causes the remnant to hurry away from the supernova remnant. We see this with some neutron stars, the place we observe the neutron star leaving the remnant at speeds of more than 800 kilometers per second. We aren’t totally certain what causes such massive natal kicks, however they aren’t unusual. One would assume the identical factor might occur for stellar black holes. In reality, given the higher depth of a black-hole forming supernova, you would possibly assume the kick can be even bigger. However current observations recommend that generally a stellar black gap can type with hardly any kick in any respect.
The observations concentrate on a black gap often known as V404 Cygni. It has a mass about 10 instances that of the Solar and is about 8,000 light-years away. Additionally it is a microquasar. There’s a small star that orbits V404 so intently that materials is captured by the black gap. The captured materials has created an accretion disk and jets much like these fashioned by supermassive black holes in distant galaxies. It was found in 1938 and is definitely noticed in each seen and x-rays. With an honest telescope, you could possibly even observe it out of your yard. Evidently, V404 has been fairly nicely studied.
However this new work discovered one thing new. The staff recognized a companion star orbiting the shut binary. The star has been identified for some time, however it wasn’t till we had detailed observations from the Gaia spacecraft that the staff might show it orbits the opposite two. It takes 70,000 years for the distant companion to make a single orbit, however it’s gravitationally certain to the opposite two. So V404 Cygni is a triple system, not a binary one. Which is a bit unusual. When the black gap fashioned, it ought to have been kicked away from the system. The shut companion might have held on, however the distant companion shouldn’t nonetheless be certain. So what offers?
When the staff appeared on the dynamics of the system, they discovered the natal kick of the black gap might have been no bigger than 5 km/s. In astronomical phrases, that’s primarily nothing. Subsequently, V404 should have had no natal kick. If it fashioned from a supernova explosion, that might be unlikely. To determine this thriller, the staff checked out varied fashions which may produce such a system. Every part from extremely symmetric supernova explosions to direct collapse fashions the place the black gap fashioned slowly and quietly slightly than with a single massive growth. It seems the quiet strategy is the almost definitely. It appears V404 steadily collected materials from its shut companion till it simply collapsed to turn into a black gap, and it did so quietly sufficient for the third companion to go alongside for the experience.
Reference: Burdge, Kevin B., et al. “The black hole low mass X-ray binary V404 Cygni is part of a wide hierarchical triple, and formed without a kick.” arXiv preprint arXiv:2404.03719 (2024).
