Upper Limits on Variability of the Crab Flux (2-50 keV)

Details Upper Limits on Variability of the Crab Flux (2-50 keV) Upper Limits on Variability of the Crab Flux (2-50 keV)

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2858....1m&link_type=abstract

The Astronomer's Telegram, #2858

Astronomy and Astrophysics

Astronomy

6

X-Ray, Gamma Ray, Neutron Stars, Pulsars, Transients

Scientific paper

We follow up on a report by AGILE of increased gamma-ray flux from the Crab nebula (Tavani et al. 2010, ATEL #2855). The BAT team routinely monitors the Hard X-ray intensity of the Crab nebula. In the time period in question (2010-09-19 to 2010-09-21) the BAT does not detect variations of more than 5.5% (15-50 keV; 1-sigma) from the mean level. We also note that there are no apparent intensity variations detected by the RXTE All-Sky Monitor (2-12 keV) in the same time range.

Affiliated with

Also associated with

No associations

Rating

Upper Limits on Variability of the Crab Flux (2-50 keV) 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 Upper Limits on Variability of the Crab Flux (2-50 keV), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Upper Limits on Variability of the Crab Flux (2-50 keV) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-774293