Mapping the Intergalactic Medium in Chandra Deep Fields

Details Mapping the Intergalactic Medium in Chandra Deep Fields Mapping the Intergalactic Medium in Chandra Deep Fields

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...209.7707p&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #77.07; Bulletin of the American Astronomical Society, V

Astronomy and Astrophysics

Astronomy

Scientific paper

The warm/hot intergalactic medium (WHIM) in the cosmic web may help solve the missing baryon problem. Recent observations of the cosmic X-ray background (CXB) in the Chandra Deep Fields North and South by Hickox and Markevitch (2005) compel us to revisit earlier theoretical predictions for the WHIM integrated spectrum and flux distribution. We use a new higher resolution large scale simulation which includes the effects of galactic superwind feedback to create maps which reproduce the spatial and energy resolution, and pixel selection criteria of the Chandra fields. We compare these statistically with the CXB they obtain and to predict the signature of this important baryon reservoir in the CCF of the CXB with the galaxy distribution.

Affiliated with

Also associated with

No associations

Rating

Mapping the Intergalactic Medium in Chandra Deep Fields does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Mapping the Intergalactic Medium in Chandra Deep Fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mapping the Intergalactic Medium in Chandra Deep Fields will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1157971