A wierd flash of gamma rays from area is upending our concepts on stellar collisions. This gamma ray burst (GRB) appears to have come from two stars smashing collectively close to the centre of an previous galaxy, a vastly totally different origin from different occasions prefer it.
There are two kinds of GRBs: brief ones, which final two seconds or much less, and lengthy ones. Long GRBs are usually thought to happen when a large star explodes in a supernova, whereas most brief GRBs appear to return from binary neutron stars – extremely dense stellar corpses – smashing collectively.
The one in query, referred to as GRB191019A, was a lengthy GRB, however nonetheless appears to have come from two dead stars, or presumably a star and a black gap, colliding.
Anya Nugent at Northwestern University in Illinois and her colleagues used information from six observatories to dig into the main points of highly effective blast, which occurred in 2019 and lasted a little over one minute. They discovered that the burst got here from near the centre of a galaxy about 3.3 billion gentle years away, however noticed no trace of the supernova anticipated to be required for a lengthy GRB.
Those supernovae are likely to be extra widespread in younger, lively galaxies, however this galaxy is extraordinarily previous. Most of its large stars have already gone by the primary part of their lives and advanced into neutron stars, white dwarfs and black holes. Because GRB191019A got here from so near the centre of its galaxy, the place these stellar corpses whiz round in abundance, the researchers discovered that it’s almost definitely two of them collided to create this blast of radiation.
We’ve by no means seen such concrete proof of two stars colliding in this sort of surroundings earlier than, says Nugent. “With binary neutron stars, we think they’re born together, they die together, and eventually merge together,” she says. “This is our first observational evidence that these stars weren’t born together: they were born, they died, and eventually in their death they found each other.”
But it’s nonetheless puzzling how one in all these stellar collisions may produce a full minute of radiation as an alternative of the short flare typical of brief GRBs.
“The idea that long GRBs could come from mergers is really throwing a lot of astronomers for a loop – we still need to figure out how we could even be getting this much emission,” says Nugent. The crew hopes that recognizing extra GRBs like this might assist unravel the thriller.
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