Limits on O VII Emission from Local and Halo Sources of the ROSAT 1/4-keV Diffuse Background

Details Limits on O VII Emission from Local and Halo Sources of the ROSAT 1/4-keV Diffuse Background Limits on O VII Emission from Local and Halo Sources of the ROSAT 1/4-keV Diffuse Background

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21541524s&link_type=abstract

American Astronomical Society, AAS Meeting #215, #415.24; Bulletin of the American Astronomical Society, Vol. 42, p.264

Astronomy and Astrophysics

Astronomy

Scientific paper

We have correlated O VII intensity in nine fields observed with Suzaku with the local and halo components of the ROSAT R12 (1/4-keV) band X-ray intensity, with the goal of finding upper limits for the temperatures and recombination rates of the 1/4-keV-emitting material. While the number of directions is limited, the results strongly indicate that very little of the observed O VII is produced by this material. This work was supported by the National Science Foundation's REU
program and the Department of Defense's ASSURE program through NSF
Award AST-0453442.

Affiliated with

Also associated with

No associations

Rating

Limits on O VII Emission from Local and Halo Sources of the ROSAT 1/4-keV Diffuse Background 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 Limits on O VII Emission from Local and Halo Sources of the ROSAT 1/4-keV Diffuse Background, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Limits on O VII Emission from Local and Halo Sources of the ROSAT 1/4-keV Diffuse Background will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-966341