File:M82 - Noao0404a.jpg
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[edit]DescriptionM82 - Noao0404a.jpg |
English: Starburst Galaxy M82
Credit: Mark Westmoquette (University College London), Jay Gallagher (University of Wisconsin-Madison), Linda Smith (University College London), WIYN//NSF, NASA/ESA |
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Date | May 21, 2004 | ||||
Source | https://noirlab.edu/public/images/noao0404a/ | ||||
Author |
Credit: Mark Westmoquette (University College London), Jay Gallagher (University of Wisconsin-Madison), Linda Smith (University College London), WIYN//NSF, NASA/ESA |
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current | 22:37, 14 November 2021 | 2,672 × 2,940 (723 KB) | Fabian RRRR (talk | contribs) | == {{int:filedesc}} == {{Information |description={{en|1='''Starburst Galaxy M82 This image is a color-coded picture of the archetypal starburst galaxy M82. It shows the horizontal stellar disk of the galaxy, which harbors its active star formation, and a perpendicular supergalactic wind of ionized gas powered by the energy released in the starburst. To make this image, data from the WIYN 3.5-meter telescope on Kitt Peak were combined with data from the WFPC2 camera on the Hubble Space Tele... |
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Credit/Provider | Mark Westmoquette (University College London), Jay Gallagher (University of Wisconsin-Madison), Linda Smith (University College London), WIYN//NSF, NASA/ESA |
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Date and time of data generation | 00:00, 21 May 2004 |
JPEG file comment | cover photo nl78 This image is a color-coded picture of the archetypal starburst galaxy M82. It shows the horizontal stellar disk of the galaxy, which harbors its active star formation, and a perpendicular supergalactic wind of ionized gas powered by the energy released in the starburst. To make this image, data from the WIYN 3.5-meter telescope on Kitt Peak were combined with data from the WFPC2 camera on the Hubble Space Telescope. Purple represents emission in ionized hydrogen (H?) and ionized nitrogen, and the green is ionized sulfur in the WIYN data. In the HST image, these colors refer to H? and nitrogen separately. These data are being used in a study of the connection between structures within M82 and its galactic superwind. This image was first presented at the ÒEssential Science in HubbleÕs Final YearsÓ symposium, held 3Ð6 May 2004 at the Space Telescope Science Institute. The WIYN 3.5-meter and 0.9-meter telescopes on Kitt Peak are operated by a consortium of the University of Wisconsin, Indiana University, Yale University, and the National Optical Astronomy Observatory (NOAO). Image Credit: Mark Westmoquette (University College London), Jay Gallagher (University of Wisconsin-Madison), Linda Smith (University College London), WIYN/NSF, NASA/ESA. |
Keywords | M82 |
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IIM version | 2 |