Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3530....1m&link_type=abstract
The Astronomer's Telegram, #3530
Astronomy and Astrophysics
Astronomy
X-Ray, Neutron Star, Soft Gamma-Ray Repeater, Pulsar
Scientific paper
The MAXI/GSC detected an enhanced X-ray emission from a position consistent with 4U 0142+61 during the scan transit of 53 seconds centered at 2011-07-29 11:23:15 (UT). The scan started 214 seconds later than the Swift/BAT trigger of a short burst from this source (GCN 12209). The GSC light curve during the scan transit showed no significant spiky structure and the averaged X-ray flux was 69 +- 16 mCrab in the 4-10 keV band.
Hiroi Kazuo
Ishikawa Masaharu
Kawai Nobuyuki
Kimura Masahiro
Kitayama Hiroki
No associations
LandOfFree
MAXI GSC detection of an enhanced X-ray emission from Anomalous X-ray Pulsar 4U 0142+61 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 detection of an enhanced X-ray emission from Anomalous X-ray Pulsar 4U 0142+61, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and MAXI GSC detection of an enhanced X-ray emission from Anomalous X-ray Pulsar 4U 0142+61 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1021813