File:Messier 90 - HST.png

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Aprašymas

Also known as M90 or Messier 90, this spiral galaxy exhibits less star formation than usual due to a phenomenon called ram pressure stripping. Gas that could have collapsed to form stars was instead stripped away as the galaxy moved through the intracluster medium between galaxies. Space may be mostly empty, but a galaxy moving fast enough through it can feel it.

This galaxy was observed as part of the wonderful PHANGS-HST. archive.stsci.edu/proposal_search.php?mission=hst&id=...

Red: WFC3/UVIS F814W Green: WFC3/UVIS F555W WFC3/UVIS F438W+F336W

North is 18.79° counter-clockwise from up.
Data
Šaltinis NGC 4569
Autorius Judy Schmidt from USA

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This image was originally posted to Flickr by geckzilla at https://flickr.com/photos/54209675@N00/49652791637. It was reviewed on 2020 m. kovo 14 d. by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0.

2020 m. kovo 14 d.

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Data/LaikasMiniatiūraMatmenysNaudotojasPaaiškinimas
dabartinis21:51, 12 kovo 2020Versijos 21:51, 12 kovo 2020 miniatiūra4 073 × 3 961 (33,31 MiB)Fabian RRRR (aptarimas | indėlis)=={{int:filedesc}}== {{Information |Description=Also known as M90 or Messier 90, this spiral galaxy exhibits less star formation than usual due to a phenomenon called ram pressure stripping. Gas that could have collapsed to form stars was instead stripped away as the galaxy moved through the intracluster medium between galaxies. Space may be mostly empty, but a galaxy moving fast enough through it can feel it. This galaxy was observed as part of the wonderful PHANGS-HST. [https://archive.sts...

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