Fayl:Arp 27 - NGC 3631.png

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Asl fayl(4 264 × 3 870 piksel, fayl hajmi: 85,91 MB, MIME tipi: image/png)

Ushbu fayl Vikiomborga yuklangan boʻlib, boshqa loyihalarda ham qoʻllanilishi mumkin. Uning tavsif sahifasidan olingan maʼlumot quyida keltirilgan.

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Taʼrif

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
Sanasi
Manba Arp 27 / NGC 3631
Muallif solomon from USA

Litsenziyalash

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atribut
This file is licensed under the Creative Commons Attribution 2.0 Generic license.
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  • ulashishga – ishlanmani nusxalash, tarqatish va uzatish
  • remiks qilishga – ishni moslashtirishga
Quyidagi shartlar asosida:
  • atribut – Siz tegishli litsenziyaga havolani taqdim etishingiz va oʻzgartirishlar kiritilganligini koʻrsatishingiz kerak. Siz buni har qanday oqilona yoʻl bilan qilishingiz mumkin, lekin litsenziar Sizni yoki Sizning foydalanishingizni ma'qullashini taklif qiladigan tarzda emas.
This image was originally posted to Flickr by theantarcticsun at https://flickr.com/photos/131716393@N07/31075307697 (archive). It was reviewed on 26 Sentyabr 2019 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0.

26 Sentyabr 2019

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23 Noyabr 2018

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90 085 313 Bayt

3 870 piksel

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4 264 piksel

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Sana/VaqtMiniaturaOʻlchamlariFoydalanuvchiIzoh
joriy20:36, 26-Sentyabr 201920:36, 26-Sentyabr 2019 dagi versiya uchun tasvir4 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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