File:Eso0304c.tif
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DescriptionEso0304c.tif |
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. |
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Date | 16 January 2003 (Release) | ||||
Source | https://www.eso.org/public/images/eso0021f/ | ||||
Author | Credit: ESO | ||||
Permission (Reusing this file) |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 07:00, 5 December 2016 | ![]() | 3,028 × 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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Width | 3,028 px |
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Height | 2,202 px |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 1 |
Horizontal resolution | 360 dpi |
Vertical resolution | 360 dpi |
Data arrangement | chunky format |
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