Chandra Position and Optical/IR Identification for IGR J11435-6109

Details Chandra Position and Optical/IR Identification for IGR J11435-6109 Chandra Position and Optical/IR Identification for IGR J11435-6109

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1231....1t&link_type=abstract

The Astronomer's Telegram, #1231

Astronomy and Astrophysics

Astronomy

3

Infra-Red, Optical, X-Ray, Binaries, Neutron Stars, Pulsars

Scientific paper

IGR J11435-6109 is a hard X-ray source that is located within 0.7 degrees of the Galactic plane. X-ray pulsations with a period of 161.76 seconds have been detected from this source (ATELs #359 and #362) as well as a long-term X-ray modulation with a period of 52.36 days (ATELs #359 and #362 and Wen et al. 2006). These periodicities strongly suggest that the system is a High Mass X-ray Binary (HMXB) with a neutron star orbiting its companion with an orbital period of 52.36 days.

Affiliated with

Also associated with

No associations

Rating

Chandra Position and Optical/IR Identification for IGR J11435-6109 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 Chandra Position and Optical/IR Identification for IGR J11435-6109, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chandra Position and Optical/IR Identification for IGR J11435-6109 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-956352