File:NGC 4536 ...from STIS.png

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STIS is Hubble's spectrograph. It usually doesn't make images*. Sometimes, though, it does, and I feel lucky when I find them, because they can really be quite good. The colors are cobbled together from a variety of sources other than STIS. Some from WFPC2, others from WFC3. Color data wasn't available for the whole frame, so the top corners are monochrome. Still looks pretty good. Even got some H-alpha data in there.

There is a lot of dust in this nucleus, and apparently a lot of star formation going on. We can easily see the pink fluffs of clouds which are associated with the processes of star formation.

  • Phil Plait tells me it makes a lot of images. I must be missing something when browsing the archive. I will try to be more watchful in the future.

Data from the following proposals were utilized: archive.stsci.edu/proposal_search.php?mission=hst&id=... archive.stsci.edu/proposal_search.php?mission=hst&id=... archive.stsci.edu/proposal_search.php?mission=hst&id=...

Color channels are generally: Red: F814W and F658N Green: F675W Blue: F555W Luminosity: Broadband optical light from STIS

North is 140.3° clockwise from up.
Date
Source NGC 4536 ...from STIS!
Author Judy Schmidt from Fresh Meadows, NY, USA

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This image was originally posted to Flickr by geckzilla at https://flickr.com/photos/54209675@N00/31484738073. It was reviewed on 14 January 2017 by FlickreviewR and was confirmed to be licensed under the terms of the cc-by-2.0.

14 January 2017

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current13:43, 14 January 2017Thumbnail for version as of 13:43, 14 January 2017980 × 987 (1.6 MB)Fabian RRRR (talk | contribs){{Information |Description=STIS is Hubble's spectrograph. It usually doesn't make images*. Sometimes, though, it does, and I feel lucky when I find them, because they can really be quite good. The colors are cobbled together from a variety of sources o...

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