File:Hubble Sees Detailed New Structures in Three Radio Galaxies (1995-30-317).jpg

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Hubble_Sees_Detailed_New_Structures_in_Three_Radio_Galaxies_(1995-30-317).jpg(800 × 500 pixels, file size: 65 KB, MIME type: image/jpeg)

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English: These Hubble Space Telescope images, combined with radio maps produced by the Very Large Array Radio Interferometer (blue contour lines), show surprisingly varied and intricate structures of gas and stars that suggest the mechanisms powering radio galaxies are more complex than thought previously. The bizarre, never before seen detail may be a combination of light from massive star forming regions, small satellite dwarf galaxies, and bow shocks caused by jets of hot gas blasted out of the galaxies' cores by suspected black holes.
Date 7 August 1995 (upload date)
Source Hubble Sees Detailed New Structures in Three Radio Galaxies
Author M. Longair (Cambridge University, England), NASA, and NRAO
Keywords
InfoField
Galaxies; Active Galaxies/Quasars

Licensing[edit]

Public domain This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.
The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org.
For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.

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current17:04, 20 April 2024Thumbnail for version as of 17:04, 20 April 2024800 × 500 (65 KB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://stsci-opo.org/STScI-01EVVG4K028PS08DQC0MSTN262.jpg via Commons:Spacemedia

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