The hard X-ray source IGR J13550-7218 is a new AGN

Details The hard X-ray source IGR J13550-7218 is a new AGN The hard X-ray source IGR J13550-7218 is a new AGN

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2563....1l&link_type=abstract

The Astronomer's Telegram, #2563

Astronomy and Astrophysics

Astronomy

1

X-Ray, Gamma Ray, Agn, Stars

Scientific paper

With reference to the recent detection of the soft X-ray counterpart of the hard X-ray source IGR J13550-7218 (Rodriguez et al. 2010, Atel #2557) we note that the XRT position is compatible with the compact radio source SUMSS J135512.53-721916.2 listed in the Sydney University Molonglo Sky Survey (Mauch et al. 2003, MNRAS, 342, 1117) with a 36 cm flux of 18.8 mJy (see attached figure). This radio source is most likely associated to PMN J1355-7219 or at least provide a great fraction of its 25 mJy flux at 6 cm (Wright et al.

Affiliated with

Also associated with

No associations

Rating

The hard X-ray source IGR J13550-7218 is a new AGN 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 The hard X-ray source IGR J13550-7218 is a new AGN, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The hard X-ray source IGR J13550-7218 is a new AGN will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1311162