File:Quasar J1507+3129 (13851306373).png

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Captions

Captions

Quasar host galaxies are hard to image. They're very far away and the quasar itself is very bright. Take a look at 3C 273 and you'll see what I mean.

Summary

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Description
English: Quasar host galaxies are hard to image. They're very far away and the quasar itself is very bright. Take a look at 3C 273 and you'll see what I mean. The quasar's glow (which astronomers dryly but more accurately refer to as a point spread function) covers up the galaxy itself. Another image in the Wikipedia article shows 3C 273 with the glow subtracted, revealing the galaxy.

Anyway, this one is different. I didn't have to do that, thankfully. I will point to the quasar. It is not the obvious bright spiral galaxy to the lower right. Look up and to the left of that bright spiral and find the merging galaxies. You can see the quasar itself as a bright point in the right side partition of the colliding masses. There is a lot of dust which is reddening the quasar. Hubble's view of things like this is not as good as it could be. This is a job for an infrared telescope! With a small amount of luck and the efforts of many scientists and engineers, JWST will perform this task. Maybe even this very quasar will be looked at. It will be interesting to combine the data sets from both Hubble and JWST one day.

Red: ACS/WFC WFC1-1K F814W (j95w11010_drz) Green: Pseudo Blue: ACS/WFC WFC1-1K F475W (j95w11020_drz)

North is NOT up. It is 22° clockwise from up.
Date Taken on 13 April 2014, 22:53:27
Source Quasar J1507+3129
Author geckzilla
Flickr sets
InfoField
all astronomy; Hubble Processing
Flickr tags
InfoField
hubble; qsoj15073129; quasar; hst; reddened; hla; dust

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This image was originally posted to Flickr by geckzilla at https://flickr.com/photos/54209675@N00/13851306373. It was reviewed on 24 February 2024 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0.

24 February 2024

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