INTEGRAL Monitoring of the Bright Neutron Star Low Mass X-Ray Binaries: Preliminary Results on GX 17+2

Details INTEGRAL Monitoring of the Bright Neutron Star Low Mass X-Ray Binaries: Preliminary Results on GX 17+2 INTEGRAL Monitoring of the Bright Neutron Star Low Mass X-Ray Binaries: Preliminary Results on GX 17+2

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.552..369p&link_type=abstract

Proceedings of the 5th INTEGRAL Workshop on the INTEGRAL Universe (ESA SP-552). 16-20 February 2004, Munich, Germany. Scientific

Computer Science

1

Scientific paper

GX 17+2 is a bright Neutron Star Low Mass X-ray Binary. Albeit significant results were obtained from previous campaigns, many open points still remain in the understanding of such a source, in particular the origin (thermal or not) of the hard component and its behavior with the spectral state. INTEGRAL offers the opportunity to reduce these ambiguities. Com- bining data from JEM-X, IBIS and SPI to provide a complete soft to hard energy coverage, we report preliminary results based on the first year Core Pro- gram observations of GX 17+2 .

Affiliated with

Also associated with

No associations

Rating

INTEGRAL Monitoring of the Bright Neutron Star Low Mass X-Ray Binaries: Preliminary Results on GX 17+2 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 INTEGRAL Monitoring of the Bright Neutron Star Low Mass X-Ray Binaries: Preliminary Results on GX 17+2, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and INTEGRAL Monitoring of the Bright Neutron Star Low Mass X-Ray Binaries: Preliminary Results on GX 17+2 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-839908