X-ray emission in the Abell 2597 Brightest Cluster Galaxy

None
Share this:
Embed*
Cite this:

Tremblay, Grant (2012): X-ray emission in the Abell 2597 Brightest Cluster Galaxy. figshare.

http://dx.doi.org/10.6084/m9.figshare.97271
Retrieved 12:08, Oct 31, 2014 (GMT)

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

Links

Comments (0)

You must be logged in to post comments.

Cite "Filename"

Place your mouse over the citation text to select it

Embed "X-ray emission in the Abell 2597 Brightest Cluster Galaxy"

Place your mouse over the embed code to select and copy it

Claim article

You claim request was sent. I will be handled in the next 24 hours.

Close window

Feedback

We appreciate all your comments, questions, suggestions or gratitude.

Login

The username or password entered are wrong.

Reset password

Your password will be sent to your registered e-mail address.

Create account

I agree to the Terms & Conditions *