Wide band observation of the neutron star X-ray binary GS1826-238 with Suzaku

Details Wide band observation of the neutron star X-ray binary GS1826-238 with Suzaku Wide band observation of the neutron star X-ray binary GS1826-238 with Suzaku

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010fym..confp..22n&link_type=abstract

"The First Year of MAXI: Monitoring Variable X-ray Sources", Poster Presentations, 4th International MAXI Workshop held November

Statistics

Scientific paper

We report on simultaneous X-ray (Suzaku) and radio (ATCA) observations of the low mass X-ray binary GS 1826-238 which has resemble spectrum like black hole binaries. Suzaku observed this source on 21-23 Oct. 2009 for a net exposure of about 100 ksec, while the ATCA radio telescope observed it with 5 and 9 GHz on 22 Oct. for 12 hours. Unfortunately, we did not detect radio counter parts with 3 sigma upper limits of 0.09 mJy and 0.12 mJy in 5 and 9 GHz respectively. Suzaku has successfully obtained a broadband X-ray energy spectrum in the 0.5-120 keV range with a good statistics. The averaged spectrum can be well explained by a blackbody plus a power law with an exponential cutoff of 51 keV. Comparison with the low/hard state of black hole binaries will be discussed.

Affiliated with

Also associated with

No associations

Rating

Wide band observation of the neutron star X-ray binary GS1826-238 with Suzaku 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 Wide band observation of the neutron star X-ray binary GS1826-238 with Suzaku, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Wide band observation of the neutron star X-ray binary GS1826-238 with Suzaku will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1290516