File:Multiwavelength View of NGC 1300 (ALMA, VLT) (2022-007-01FRNP2ZWBJ47ECPBBBN939F3E).png
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English: This image of spiral galaxy NGC 1300 combines multiple observations to map stellar populations and gas. Radio light observed by the Atacama Large Millimeter/submillimeter Array (ALMA), represented in yellow, highlights the clouds of cold molecular gas that provide the raw material from which stars form. Data from the Very Large Telescope’s Multi Unit Spectroscopic Explorer (MUSE) instrument is represented in red and magenta, capturing the impact of young, massive stars on their surrounding gas. Visible and ultraviolet light captured by the Hubble Space Telescope highlights dust lanes in gold and very young, hot stars in blue. High-resolution infrared images from the Webb Space Telescope will help researchers identify where stars are forming behind dust and study the earliest stages of star formation in this galaxy. |
| Date | 19 January 2022 (upload date) |
| Source | Multiwavelength View of NGC 1300 (ALMA, VLT) |
| Author | SCIENCE: NASA, ESA, ESO-Chile, ALMA, NAOJ, NRAO IMAGE PROCESSING: Alyssa Pagan |
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This file is in the public domain because it was created by NASA, ESA and CSA. NASA Webb material 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/CSA is credited as the source of the material. This license does not apply if source material from other organizations is in use. The material was created for NASA by Space Telescope Science Institute under Contract NAS5-03127. Copyright statement at webbtelescope.org. For material created by the European Space Agency on the esawebb.org site, use the {{ESA-Webb}} tag. |
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| current | 00:46, 19 February 2023 | | 3,522 × 3,513 (20.57 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://stsci-opo.org/STScI-01FRNQQ4ACVYRA3QQ2X6AZDPGZ.png via Commons:Spacemedia |
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