File:Ngc1404 hst.tif
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Size of this JPG preview of this TIF file: 613 × 599 pixels. Other resolutions: 245 × 240 pixels | 491 × 480 pixels | 786 × 768 pixels | 1,047 × 1,024 pixels | 2,095 × 2,048 pixels | 3,544 × 3,465 pixels.
Original file (3,544 × 3,465 pixels, file size: 26.17 MB, MIME type: image/tiff)
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DescriptionNgc1404 hst.tif | Hubble Optical Image of NGC 1404 | ||||
Source | http://chandra.harvard.edu/photo/2008/ngc1404/more.html / http://chandra.harvard.edu/photo/2008/ngc1404/ngc1404_hst.tif | ||||
Author | Credit: NASA/STScI | ||||
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 13:40, 25 April 2016 | 3,544 × 3,465 (26.17 MB) | Fabian RRRR (talk | contribs) | {{Information |Description=Hubble Optical Image of NGC 1404 |Source=http://chandra.harvard.edu/photo/2008/ngc1404/more.html / http://chandra.harvard.edu/photo/2008/ngc1404/ngc1404_hst.tif |Date= |Author=Credit: NASA/STScI |Permission={{PD-Hubble}} |oth... |
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Image title | Chandra's X-ray image (left), obtained in 2003, shows the same field-of-view on the sky as an optical view from the Swift satellite from November 2007 (right). An X-ray source appears close, but not exactly aligned, to where the supernova was detected. A progenitor to such a Type Ia supernova has never been detected, but would provide answers to important questions about the exact configuration and trigger for these explosions. Further observations are needed to determine whether this X-ray source is the progenitor of SN 2007on. |
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Author | Chandra X-ray Observatory Center |
Width | 3,544 px |
Height | 3,465 px |
Bits per component |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 24 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop CS2 Macintosh |
File change date and time | 09:30, 30 January 2008 |
Exif version | 2.21 |
Color space | Uncalibrated |
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