Credit & Copyright: A. Hobart,
CXC
Explanation:
In the center of a swirling whirlpool of hot gas
is likely a beast that has never been seen directly: a
black hole.
Studies of the bright light emitted by the
swirling gas frequently indicate not only that a
black hole is present, but also likely attributes.
The gas surrounding GRO J1655-40, for example, has recently been found to display an unusual flickering
at a rate of 450 times a second.
Given a
previous mass estimate for the central object of seven times the mass of our Sun,
the rate of the
fast flickering can be
explained by a
black hole that is rotating very rapidly.
What physical mechanisms actually cause the flickering --
and a slower quasi-periodic oscillation (QPO) -- in
accretion disks
surrounding
black holes and
neutron stars remains a topic of much research.
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Publikacii s klyuchevymi slovami:
chernye dyry - black hole - neitronnye zvezdy - microquasar - QPO - accretion disk - akkrecionnyi disk
Publikacii so slovami: chernye dyry - black hole - neitronnye zvezdy - microquasar - QPO - accretion disk - akkrecionnyi disk | |
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