File:Eso0304c.tif

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Description

This image shows the general location of the newly discovered compact HII region with respect to a previously published Subaru Suprime-Cam image of NGC 4388. The image combines H-alpha narrow-band (hydrogen), O[III] narrow-band (oxygen), and broad-band optical V-band data. The extended pink filamentary structure in this image is due to gas ionized by the radiation from the nucleus of the galaxy. The vertical lines are caused by detector saturation of bright objects. The field of view is 11.6 x 5.0 arcmin2.

Credit: ESO

Coordinates
Position (RA):	12 25 48.13
Position (Dec):	12° 41' 39.37"
Field of view:	12.34 x 8.98 arcminutes
Orientation:	North is 1.6° right of vertical
Colours & filters Band	Wavelength	Telescope
Optical V		Subaru Telescope Suprime-Cam
Optical OIII	502 nm	Subaru Telescope Suprime-Cam
Optical H-alpha	660 nm	Subaru Telescope Suprime-Cam
.
Date 16 January 2003 (Release)
Source https://www.eso.org/public/images/eso0021f/
Author Credit: ESO
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This media was created by the European Southern Observatory (ESO).
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Date/TimeThumbnailDimensionsUserComment
current07:00, 5 December 2016Thumbnail for version as of 07:00, 5 December 20163,028 × 2,202 (12.88 MB)Fabian RRRR (talk | contribs){{Information |Description= This image shows the general location of the newly discovered compact HII region with respect to a previously published Subaru Suprime-Cam image of NGC 4388. The image combines H-alpha narrow-band (hydrogen), O[III] narrow-b...

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