Dosya:Arp 27 - NGC 3631.png

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Şınasnayış

This galaxy was observed due to a supernova - SN 2016bau. This is in Arp's catalogue as an example of a spiral galaxy with one heavy arm, but that doesn't seem to be the case for this galaxy. It's a pretty standard spiral.

The chip gap was filled with older WFPC2 data where it could be. I painted some fake data to minimise distraction where no data was available. To the left, there is also some lower resolution WFPC2 data. Quite a few cosmic rays were removed and some pretty intense sharpness/clarity adjustments were made.

Morphological type: SAc

Red: ACS/WFC F814W Green: pseudo Blue: ACS/WFC F555W

Chip-gap Red: WFPC2 F814W Green: pseudo

Blue: WFPC2 F606W
Tarix
Çıme Arp 27 / NGC 3631
Nuştekar solomon from USA

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This image was originally posted to Flickr by theantarcticsun at https://flickr.com/photos/131716393@N07/31075307697 (archive). It was reviewed on 26 Keşkelun 2019 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0.

26 Keşkelun 2019

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23 Tışrino Peyên 2018

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nıkayên20:36, 26 Keşkelun 2019Seba versiyonê 20:36, 26 Keşkelun 2019 ra4,264 - 3,870 (85.91 MB)Fabian RRRR=={{int:filedesc}}== {{Information |Description=This galaxy was observed due to a supernova - SN 2016bau. This is in Arp's catalogue as an example of a spiral galaxy with one heavy arm, but that doesn't seem to be the case for this galaxy. It's a pretty standard spiral. The chip gap was filled with older WFPC2 data where it could be. I painted some fake data to minimise distraction where no data was available. To the left, there is also some lower resolution WFPC2 data. Quite a few cosmic ra...

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