MAXI/GSC detects a quasi-regular outburst and a possible soft state transition in H 1743-322

Details MAXI/GSC detects a quasi-regular outburst and a possible soft state transition in H 1743-322 MAXI/GSC detects a quasi-regular outburst and a possible soft state transition in H 1743-322

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012atel.3842....1n&link_type=abstract

The Astronomer's Telegram, #3842

Astronomy and Astrophysics

Astronomy

X-Ray, Binary, Black Hole, Transient

Scientific paper

MAXI/GSC detected renewed activity from the Galactic black hole candidate H 1743-322 on December 22, 2011 (MJD 55917) with a flux of 29±8 mCrab in the 4-10 keV band. The source was slightly visible in an image on December 19, but solar X-rays and invisible areas of detectors did not allow us to confirm the source activity until December 22. The 2-20 keV flux has increased since December 22, and the spectrum became soft on December 31.

Affiliated with

Also associated with

No associations

Rating

MAXI/GSC detects a quasi-regular outburst and a possible soft state transition in H 1743-322 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 MAXI/GSC detects a quasi-regular outburst and a possible soft state transition in H 1743-322, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and MAXI/GSC detects a quasi-regular outburst and a possible soft state transition in H 1743-322 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-908118