File:Outflow from M82 galaxy.jpg
Outflow_from_M82_galaxy.jpg (426 × 426 pixels, file size: 46 KB, MIME type: image/jpeg)
Summary[edit | edit source]
Shown in red is the outflow from the galaxy M82 of polycyclic aromatic hydrocarbons (PAH)s embedded in a gaseous wind propelled out of the galaxy by hot stars in the stellar disk (blue).
Licensing[edit | edit source]
Description |
Shown in red is the outflow of polyaromatic hydrocarbons (PAH)s embedded in a gaseous wind propelled out of the galaxy by hot stars in the stellar disk (blue). |
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Source |
The image from the Spitzer infrared telescope appears in a web white paper at url=http://astrophysics.gsfc.nasa.gov/cosmology/spirit/FIR-SIM_Crosscutting_White_Paper.pdf. |
Date |
May 28-30, 2008 |
Author |
Martin Harwit, George Helou, Lee Armus, C. Matt Bradford, Paul F. Goldsmith, Michael Hauser, David Leisawitz, Daniel F. Lester, George Rieke, and Stephen A. Rinehart |
Permission (Reusing this file) |
Fair Use, as the image is in a White Paper published by the NASA Goddard Space Flight Center it is most likely Public Domain.
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File history
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 03:15, 11 February 2014 | 426 × 426 (46 KB) | Marshallsumter (discuss | contribs) | Shown in red is the outflow from the galaxy M82 of polycyclic aromatic hydrocarbons (PAH)s embedded in a gaseous wind propelled out of the galaxy by hot stars in the stellar disk (blue). Category:Galaxies |
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