Radio Properties of the Hard X-ray transient IGR J18175-1530

Details Radio Properties of the Hard X-ray transient IGR J18175-1530 Radio Properties of the Hard X-ray transient IGR J18175-1530

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1289....1c&link_type=abstract

The Astronomer's Telegram, #1289

Astronomy and Astrophysics

Astronomy

Radio, X-Ray, Gamma Ray, A Comment, Agn, Binaries, Black Holes, Neutron Stars, Pulsars, Transients, Variables

Scientific paper

In response to the discovery of the new hard X-ray transient IGR J18175-1530 and its possible association with the radio source GPSR5 15.308+0.226 (hereafter GPS15.3) by Paizis et al. (ATEL #1248), radio images of the field from MAGPIS and NVSS were examined. The 1.4 GHz MAGPIS image (5.4" x 6.2" resolution; Helfand et al. 2006 AJ 131, 2525) shows GPS15.3 to be a discrete 30 mJy (18 mJy peak) source, whereas the lower resolution (45") 1.4 GHz NVSS map shows a tail of emission extending to the northeast with a 7 mJy peak that is slightly offset (to the east) of GPS15.3.

Affiliated with

Also associated with

No associations

Rating

Radio Properties of the Hard X-ray transient IGR J18175-1530 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 Radio Properties of the Hard X-ray transient IGR J18175-1530, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio Properties of the Hard X-ray transient IGR J18175-1530 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-736816