Chandra Monitoring Observations of 1E 1048.1-5937: A Prolonged Flux Enhancement

Details Chandra Monitoring Observations of 1E 1048.1-5937: A Prolonged Flux Enhancement Chandra Monitoring Observations of 1E 1048.1-5937: A Prolonged Flux Enhancement

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1076....1g&link_type=abstract

The Astronomer's Telegram, #1076

Astronomy and Astrophysics

Astronomy

4

X-Ray, Neutron Stars, Soft Gamma-Ray Repeaters

Scientific paper

In 2007 March Dib et al. 2007 reported a pulsed flux enhancement and glitch from the Anomalous X-ray pulsar (AXP) 1E 1048.1-5937 (see ATEL #1041, ATEL #1043). We initiated four Chandra ToOs to monitor the source, with the most recent being on 2007 April 28. Post-glitch, the source continues to be bright with an unabsorbed 2-10 keV flux of ~3.6x10^-11 erg cm^2 s^-1 in all Chandra observations. Note that the quiescent flux of this source is ~4.7x10^-12 erg cm^2 s^-1.

Affiliated with

Also associated with

No associations

Rating

Chandra Monitoring Observations of 1E 1048.1-5937: A Prolonged Flux Enhancement 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 Chandra Monitoring Observations of 1E 1048.1-5937: A Prolonged Flux Enhancement, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chandra Monitoring Observations of 1E 1048.1-5937: A Prolonged Flux Enhancement will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-765790