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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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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
Publications with keywords: black hole - microquasar - QPO - accretion disk
Publications with words: black hole - microquasar - QPO - accretion disk
See also:
- APOD: 2024 November 24 Á Journey to the Center of the Galaxy
- APOD: 2024 October 1 Á Porphyrion: The Longest Known Black Hole Jets
- APOD: 2024 June 16 Á Animation: Black Hole Destroys Star
- Simulation: Two Black Holes Merge
- The Galaxy, the Jet, and a Famous Black Hole
- APOD: 2024 May 8 Á Visualization: A Black Hole Accretion Disk
- APOD: 2024 May 7 Á Black Hole Accreting with Jet