Tuesday, December 6, 2011

Space / Astronomy: What's Hot Now: Giant Disk of Cold Gas and Dust Fuels Possible Black Hole at Core of NGC 4261

Space / Astronomy: What's Hot Now
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Giant Disk of Cold Gas and Dust Fuels Possible Black Hole at Core of NGC 4261
Dec 6th 2011, 17:05

Astronomers using NASA's Hubble Space Telescope (HST) have gotten their best look yet at the disk of material that surrounds and is being pulled into a suspected black hole.

The disk is at the core of a galaxy in the Virgo Cluster 45 million light-years from Earth. Dr. Walter Jaffe of Leiden Observatory in The Netherlands said the disk is tipped about 60 degrees â€" enough to provide astronomers with a clear view of the galaxy's bright hub.

The nucleus is probably the home of a black hole with a mass 10 million times that of our Sun, Jaffe said. "This is our best view to date of the immediate surrounding of the nucleus of an active galaxy," the name given galaxies that emit especially strong radiation indicating that they harbor powerful energy sources.

This is the first case where we can follow the disk's gas in an orderly way down to the immediate environment of the black hole, said co-investigator Dr. Holland Ford of The Johns Hopkins University in Baltimore, Maryland.

The observations made with the Wide Field/Planetary Camera (WFIPC) in PC mode make a strong contribution to mounting evidence for the existence of black holes in the universe, the two astronomers said.

A black hole is a theoretical object which forms after a massive stars collapses. The star's matter is so densely compacted that it has a powerful gravitational pull that traps all matter that comes near it.

Black holes are to date theoretical because their gravitational pull is so great that not even light can escape. Therefore, they cannot be seen. Astronomers can only infer a black hole's existence by its gravitational influence on the motion of stars and other material near it.

The galaxy, designated NGC 4261, was selected for study because it is one of the brightest in the Virgo Cluster.

The galaxy is unremarkable in visible light, said Jaffe. "However, observations with radio telescopes show a pair of opposed jets emanating from the nucleus and spanning a distance of 88,000 light-years." Spectroscopic data (from the Observatory del Roque de los Muchachos in the Canary Islands) show ionized gas in the nucleus moving at speeds approaching several million miles an hour, or one percent of the speed of light.

Most astronomers believe both phenomena, which have been seen earlier in radio galaxies and quasars (active nuclei of remote galaxies), to be caused by material being swallowed by massive black holes hiding in the nuclei of large galaxies, said Ford.

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