The star may represent a brief transitory stage in the evolution of
extremely massive stars.
«Many astronomers, including our group, have already provided a great deal of evidence that long - duration gamma - ray bursts (those lasting more than two seconds) are produced by the collapse of
extremely massive stars.
Current theories suggest that the seeds of these black holes were the result of either the growth and collapse of the first generation of stars in the Universe; collisions between stars in dense stellar clusters; or the direct collapse of
extremely massive stars in the early Universe.
«People most often associate stellar explosions with ancient stars, like a nova eruption on the surface of a decaying star or the even more spectacular supernova death of
an extremely massive star,» Bally says.
Not exact matches
The
extremely strong gravity of a
massive neutron
star in orbit with a companion white dwarf
star puts competing theories of gravity to a test more stringent than any available before
Measuring the proportion of
massive stars is
extremely difficult — primarily because of their scarcity — and there are only a handful of places in the local Universe where this can be done.
For the last few years, he has studied a gaggle of
extremely fast - moving
stars, stellar runaways that were long ago flung out of the Milky Way by the
massive black hole at its center.
Bursts probably occur after a hypernova, an
extremely rare explosion of a
star so
massive it can barely support its own bulk.
The galaxies — which would appear as flat, rotating disks — are brimming with
extremely bright and
massive blue
stars.
Extremely bright exploding
stars, called superluminous supernovae, and long gamma ray bursts also occur in this type of galaxy, he noted, and both are hypothesized to be associated with
massive, highly magnetic and rapidly rotating neutron
stars called magnetars.
When a
massive star goes supernova, its core collapses into an
extremely compact object: either a dense neutron
star or a black hole.
An ancient
star a mere thousand light - years from Earth bears chemical elements that may have been forged by the death of a
star that was both
extremely massive and one of the first to arise after the big bang.
Massive stars that collapse upon themselves and end their lives as black holes, like the pair LIGO detected, are
extremely rare, O'Shaughnessy said.
The discovery is «
extremely important in terms of understanding the evolution of the most
massive stars,» says x-ray astronomer Michael Corcoran of NASA's Goddard Space Flight Center in Greenbelt, Maryland.
Two teams of astronomers led by researchers at the University of Cambridge have looked back nearly 13 billion years, when the Universe was less than 10 percent its present age, to determine how quasars —
extremely luminous objects powered by supermassive black holes with the mass of a billion suns — regulate the formation of
stars and the build - up of the most
massive galaxies.
It is unfortunate, then, that some of the easiest planets to detect are the so - called hot Jupiters:
massive bodies hugging tight to their host
stars and therefore subject to
extremely high (and probably life - negating) temperatures.
Extremely turbulent environments can disrupt the normal procession of material onto a protostar, while intense radiation — from
massive nearby
stars and supermassive black holes — can blast away the parent cloud, thwarting the formation of all but the most
massive of
stars.
«The
massive stars have
extremely high winds associated with them and the winds are colliding and swirling at very high speeds, which make the gases in this environment very hot.
Both of these techniques work best when the planets are either
extremely massive or when they orbit very close to their parent
stars.
Supernovae (singular: supernova) are the rare and
extremely powerful explosions of
massive stars late in their evolutionary histories.
If so, then it's possible that most, if not all, of the galaxy's
extremely metal - poor
stars surviving to the present day originally formed as part of a binary pair, a byproduct of the formation of a
massive star.
Stars much more
massive than the Sun end their normal lives in violent supernova explosions, leaving behind an
extremely dense neutron
star.
Astronomers believe that these are spinning neutron
stars (
extremely dense objects formed from the collapse of
massive stars) with strong magnetic fields that emit radio signals in one direction.
A supernova is the name given to the birth of an
extremely bright, brilliant
star, caused by the spectacular explosion of a
massive star at the end of its life.