X-ray emission in the Abell 2597 Brightest Cluster Galaxy
Description
0.5-7 keV X-ray surface brightness map of the central brightest cluster galaxy in Abell 2597. The X-ray emission has been smoothed with an adaptive gaussian kernel, and surface brightness isocontours have been overlaid in black. East is left, North is up. From Tremblay et al. 2012b, Monthly Notices of the Royal Astronomical Society (MNRAS), 424, 1026
Comments (0)
You must be logged in to post comments.
174
views
Published on 08 Nov 2012 - 13:41 (GMT)
Filesize is 77.64 KB
Categories
Authors
Cite "Filename"
Place your mouse over the citation text to select it
Claim article
You claim request was sent. I will be handled in the next 24 hours.
Close window