«Typically, when neutron stars
accrete mass, this occurs every day or so,» Heyl says.
Not exact matches
This process, however, can not repeat indefinitely and the
accreting star will reach a
mass above which no physical pressure will prevent it from collapsing to a black hole.
As
mass is
accreted into one of the disks it loses gravitational energy.
[3] Type Ia Supernovae occur when an
accreting white dwarf in a binary star system slowly gains
mass from its companion until it reaches a limit that triggers the nuclear fusion of carbon.
Gaining a better understanding of how much
mass black holes
accrete may therefore provide new insight on how galaxies pack on the pounds, astronomers note.
Astrophysicist and co-author Lars Eric Hernquist of the Harvard - Smithsonian Center for Astrophysics in Cambridge, Massachusetts, says that a protostar could grow quickly,
accreting about 10 solar
masses within 1000 years, and reaching its full size of 100 or more times the sun's
mass in as little as 10,000 years.
Those furious feeding rates still seem to defy the black holes» supermassive size: A 100 - solar -
mass black hole
accreting at the limit should take about 800 million years to reach a billion solar
masses, even taking into account that it would eat faster as it grew.
In this theory material from the companion star is
accreted onto the white dwarf until its
mass reaches a limit, leading to a dramatic explosion.
Previous work had unified the variability in discs around black holes of different
mass ranges, but by considering not just the
mass of the object, but also its size, scientists can now add
accreting white dwarfs and proto - stars to this unified picture.
The riddle posed by super-Earths (1 — 4 Earth radii, 2 — 20 Earth
masses) is that they are not Jupiters: their core
masses are large enough to trigger runaway gas accretion, yet somehow super-Earths
accreted atmospheres that weigh only a few percent of their total
mass.
The latest research shows that the relatively small OTS44 has a disk containing more than 10 times the
mass of Earth, and that it is actively
accreting material.
Building on past observations of the white dwarf called SDSSJ1043 +0855 (the dead core of a star that originally was a few times the
mass of the Sun), which has been known to be gobbling up rocky material in its orbit for almost a decade, the team used Keck Observatory's HIRES instrument fitted to the 10 - meter Keck I telescope as well as data from the Hubble Space Telescope to measure and characterize the material being
accreted by the star.
If the white dwarf
accretes enough material to reach the Chandrasekhar limit, the maximum
mass of a stable white dwarf star (1.4 solar
mass), it will likely explode as a Type Ia supernova.
If rate of accretion depends on the
mass of the
accreting body, then the rate of the increase in
mass of that
accreting body increases quickly until all available material is taken.