Swift/XRT detection of X-ray emission from a symbiotic binary and another source in the field of IGR J17197-3010

Details Swift/XRT detection of X-ray emission from a symbiotic binary and another source in the field of IGR J17197-3010 Swift/XRT detection of X-ray emission from a symbiotic binary and another source in the field of IGR J17197-3010

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012atel.3960....1l&link_type=abstract

The Astronomer's Telegram, #3960

Astronomy and Astrophysics

Astronomy

X-Ray, A Comment

Scientific paper

We report the Swift/XRT detection of two sources in the field of IGR J17197-3010. Swift observed the field of IGR J17197-3010 for a total of 10394 s between 2010-03-05 and 2012-02-12, detecting the first source at a 6.4 sigma level with a count rate of 0.0087+/-0.0014 counts/s at the coordinates alpha = 17h 19m 51.7s and delta = -30d 02' 0.6" (with an error radius of 4.3"). These XRT coordinates are consistent with the position of a symbiotic star at alpha = 17h 19m 51.83s and delta =-30d 02m 0.3s that Massetti et al.

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