File:Phot-34b-05-fullres.jpg
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Size of this preview: 556 × 600 pixels. Other resolutions: 223 × 240 pixels | 445 × 480 pixels | 712 × 768 pixels | 950 × 1,024 pixels | 1,789 × 1,929 pixels.
Original file (1,789 × 1,929 pixels, file size: 2.62 MB, MIME type: image/jpeg)
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DescriptionPhot-34b-05-fullres.jpg |
English: The largest member of the galaxy group known as Roberts Quartet is NGC 92, a spiral Sa galaxy with an unusual appearance. One of its arms, about 100,000 light-years long, has been distorted by interactions and contains a large quantity of dust. Using this H-alpha image obtained with FORS2 on the VLT, astronomers were able to study the properties of regions of active star formation ("HII regions"). They found more than 200 of such regions in NGC 92, with a size between 500 and 1,500 light-years.
ID: phot-34b-05 Press: 34/05 Object: NGC 92 Instrument: FORS2 Size: 1789x1929 Credit: ESO |
Date | Wed 04 Feb 2009 14:10:11 CET |
Source | http://www.eso.org/gallery/v/ESOPIA/Galaxies/phot-34b-05-fullres.jpg.html |
Author | ESO |
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This file is licensed under the Creative Commons Attribution 4.0 International license.
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 19:56, 28 April 2009 | 1,789 × 1,929 (2.62 MB) | Fabian RRRR (talk | contribs) | {{Information |Description={{en|1=The largest member of the galaxy group known as Robert''s Quartet is NGC 92, a spiral Sa galaxy with an unusual appearance. One of its arms, about 100,000 light-years long, has been distorted by interactions and contains |
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Orientation | Normal |
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Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Software used | Adobe Photoshop CS3 Macintosh |
File change date and time | 14:10, 4 February 2009 |
Color space | Uncalibrated |