Swift confirms identification of RT Cru as the IGR J12349-6434 hard x-ray source

Details Swift confirms identification of RT Cru as the IGR J12349-6434 hard x-ray source Swift confirms identification of RT Cru as the IGR J12349-6434 hard x-ray source

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..591....1t&link_type=abstract

The Astronomer's Telegram, #591

Astronomy and Astrophysics

Astronomy

5

Binaries, Variables

Scientific paper

The hard x-ray source, IGR J12349-6434 and SWIFT J1234.7-6433 (BAT survey source), has been detected by Swift XRT. There is only one bright x-ray source in the BAT error circle, with an absorbed flux of 3 x 10^11 erg/cm^2/s (0.5-10 keV). The XRT position is R.A.=12h34m54.7s , Decl.=-64d33m55.6s The XRT position is 5" from the symbiotic star RT Cru within the 6" XRT error radius, confirming the suggested identification of N.

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