Flaring history of IGR J17544-2619 unveils stellar wind clumping

Details Flaring history of IGR J17544-2619 unveils stellar wind clumping Flaring history of IGR J17544-2619 unveils stellar wind clumping

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1269....1w&link_type=abstract

The Astronomer's Telegram, #1269

Astronomy and Astrophysics

Astronomy

X-Ray, Gamma Ray, Binaries, Transients

Scientific paper

To follow on ATEL#1265 and ATEL #1266 we point out that Walter & Zurita (2007, in press; astro-ph 0710.2542) have reported 8 flares of IGR J17544-2619 detected by INTEGRAL/ISGRI for a total effective exposure time (corrected for the variation of the sensitivity with off-axis angle) of about 76 days. About one flare is detected every 10 days of observation on average. IGR J17544-2619 is one of the supergiant fast X-ray transient system featuring the largest variability factor.

Affiliated with

Also associated with

No associations

Rating

Flaring history of IGR J17544-2619 unveils stellar wind clumping 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 Flaring history of IGR J17544-2619 unveils stellar wind clumping, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Flaring history of IGR J17544-2619 unveils stellar wind clumping will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-736292