Archivo de imágenes de Hubble

Hubble se acerca al doble núcleo de la galaxia de Andrómeda

A new Hubble Space Telescope image centers on the 100-million-solar-mass black hole at the hub of the neighboring spiral galaxy M31, or the Andromeda galaxy, one of the few galaxies outside the Milky Way visible to the naked eye and the only other giant galaxy in the Local Group....

Fecha
Jan 1, 2012
Misión
Hubble Space Telescope
ID de archivo
hubblesite-images-2012-04-2961-image
Por

A new Hubble Space Telescope image centers on the 100-million-solar-mass black hole at the hub of the neighboring spiral galaxy M31, or the Andromeda galaxy, one of the few galaxies outside the Milky Way visible to the naked eye and the only other giant galaxy in the Local Group.

This is the sharpest visible-light image ever made of the nucleus of an external galaxy.

The event horizon, the closest region around the black hole where light can still escape, is too small to be seen, but it lies near the middle of a compact cluster of blue stars at the center of the image. The compact cluster of blue stars is surrounded by the larger "double nucleus" of M31, discovered with the Hubble Space Telescope in 1992. The double nucleus is actually an elliptical ring of old reddish stars in orbit around the black hole but more distant than the blue stars. When the stars are at the farthest point in their orbit they move slower and give the illusion of a second nucleus.

The blue stars surrounding the black hole are no more than 200 million years old, and therefore must have formed near the black hole in an abrupt burst of star formation. Massive blue stars are so short-lived that they would not have enough time to migrate to the black hole if they were formed elsewhere.

Astronomers are trying to understand how apparently young stars were formed so deep inside the black hole's gravitational grip and how they survive in an extreme environment.

The fact that young stars are also closely bound to the central black hole in our Milky Way galaxy suggests this may be a common phenomenon in spiral galaxies.

Tod R. Lauer of the National Optical Astronomy Observatory in Tucson, Ariz., assembled this image of the nuclear region by taking several blue and ultraviolet light exposures of the nucleus with Hubble's Advanced Camera for Surveys high-resolution channel during September 2005 and February 2006, each time slightly moving the telescope to change how the camera sampled the region. By combining these pictures, he was able to construct an ultra-sharp view of the galaxy's core.

Lauer is presenting these Hubble observations today at the meeting of the American Astronomical Society in Austin, Texas.

The image of the Andromeda galaxy was taken on Jan. 13, 2001, with the WIYN/KPNO 0.9-meter Mosaic I by T. Rector and B. Wolpa of the National Optical Astronomy Observatory in Tucson, Ariz.

Credits

Hubble Image: NASA, ESA, and T. Lauer (National Optical Astronomy Observatory);
WIYN/KPNO Image: T. Rector and B. Wolpa (NOAO/AURA/NSF)

Detalles de la imagen

About The Object
Object NameM31, NGC 224, Andromeda Galaxy, and M31 Nucleus (inset image)
Object DescriptionNucleus of M31
R.A. Position00h 42m 44.0s
Dec. Position41° 16' 8.99"
ConstellationAndromeda
About The Data
Data DescriptionInset image: This image was created from Hubble data from proposal : T. Lauer (NOAO), J. Kormendy and K. Gebhardt (University of Texas, Austin), R. Bender (Universitats-Sternwarte, Munich), and R. Green (NOAO).
InstrumentWIYN/KPNO>0.9m (galaxy image), and HST>ACS/HRC (inset)
FiltersHubble Image (inset image): F330W (u) and F435W (B)
About The Image
Color InfoHubble Image (inset image): This image is a composite of separate exposures acquired by the ACS instrument on HST. Several filters were used to sample broad wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Blue: F330W (u) Orange: F435W (B)

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Ver en NASA.gov

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