Sary:NGC 4567 & 4568.png

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Here's a particular kind of galactic grouping called an overlap. It is rare to find these line-of-sight treasures in unperturbed, likely non-interacting states or early stage interacting like this.

This image is an experiment combining data from HST with William Keel's ground-based WIYN observations. I've done this a few times before, but I feel like this one turned out a bit better. You can see in the center there is a sharper area where the Hubble data were used, and outside of that is all the ground based data. The i and b filters from WIYN ended up being a pretty good match since I like to place the least noisy (HST data not necessarily the least noisy this time) and clearest data into the green channel, which is where the F606W neatly fits, with the i filter being a longer wavelength and the b being shorter.

Widefield, ground-based WIYN data were generously supplied by William Keel.

Data from the following HST proposal were used to create this image: The Nuclei of Nearby S0 and Spiral Galaxies: A PC Snapshot Imaging Survey

Red: WIYN i Green: HST/WFPC2 F606W + WIYN i+b pseudogreen Blue: WIYN b

North is up.
Daty
Loharano NGC 4567 & 4568
Mpamorona azy Judy Schmidt from USA

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Cette image a été originellement postée sur Flickr par geckzilla à l'adresse https://flickr.com/photos/54209675@N00/49736725392. Elle a été passée en revue le 5 Aprily 2020 par le robot FlickreviewR 2, qui a confirmé qu'elle se trouvait sous licence cc-by-2.0.

5 Aprily 2020

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dépeint Frantsay

mpamorona

Valeur sans élément de Wikidata

auteur ou autrice (chaîne) Frantsay : Judy Schmidt
identifiant Flickr Frantsay : 54209675@N00
URL Frantsay : https://www.flickr.com/people/54209675@N00

licence Frantsay

CC BY 2.0 Générique Frantsay

fiandohana

4 Aprily 2020

type MIME Frantsay

image/png

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ankehitriny5 Aprily 2020 à 20:32Vignette ho an'ny 5 Aprily 2020 à 20:322 182 × 2 626 (9,78 Mio)Fabian RRRR=={{int:filedesc}}== {{Information |Description=Here's a particular kind of galactic grouping called an overlap. It is rare to find these line-of-sight treasures in unperturbed, likely non-interacting states or early stage interacting like this. This image is an experiment combining data from HST with William Keel's ground-based WIYN observations. I've done this a few times before, but I feel like this one turned out a bit better. You can see in the center there is a sharper area where the H...

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