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Related: About this forum'Overweight' neutron star defies a black hole theory, say astronomers
Exclusive: Gamma-ray burst from colliding stars unexpectedly gave way to day-long sight of hypermassive body
Hannah Devlin Science correspondent
@hannahdev
Thu 10 Nov 2022 11.14 EST
An overweight neutron star has been observed by astronomers, who say the mysterious object confounds astronomical theories.
The hypermassive star was produced by the merger of two smaller neutron stars. Normally such collisions result in neutron stars so massive that they collapse into a black hole almost instantaneously under their own gravity. But the latest observations revealed the monster star hovering in view for more than a day before it faded out of sight.
Such a massive neutron star with a long life expectancy is not normally thought to be possible, said Dr Nuria Jordana-Mitjans, an astronomer at the University of Bath. It is a mystery why this one was so long-lived.
The observations also raise questions about the source of incredibly energetic flashes, known as short gamma-ray bursts (GRBs), that accompany neutron star mergers. These outbursts the most energetic events in the universe since the big bang were widely assumed to be launched from the poles of the newly formed black hole. But in this case, the observed gamma-ray burst must have emanated from the neutron star itself, suggesting that an entirely different process was at play.
More:
https://www.theguardian.com/science/2022/nov/10/overweight-neutron-star-defies-a-black-hole-theory-say-astronomers
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'Overweight' neutron star defies a black hole theory, say astronomers (Original Post)
Judi Lynn
Nov 2022
OP
Any chance that it was a partial merger with part of it breaking off but now in an extremely
cstanleytech
Nov 2022
#3
Kittycatkat
(1,734 posts)1. interesting
eppur_se_muova
(37,375 posts)2. First guess: conservation of angular momentum rules again.
It should take a while to bleed off all that orbital motion.
cstanleytech
(26,987 posts)3. Any chance that it was a partial merger with part of it breaking off but now in an extremely
tight orbit giving it the appearance of a complete merger?