Refined distance estimation of XMMU J174716.1-281048

Details Refined distance estimation of XMMU J174716.1-281048 Refined distance estimation of XMMU J174716.1-281048

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1207....1d&link_type=abstract

The Astronomer's Telegram, #1207

Astronomy and Astrophysics

Astronomy

4

X-Ray, Binaries, Neutron Stars, Transients

Scientific paper

Further INTEGRAL analysis of the radius expansion X-ray burst from the Very Faint X-ray Transient (VFXT) XMMU J174716.1-281048 (ATel #970, #972, #1078, Del Santo et al., 2007, A&A, 468, L17) results on an average (80 s) unabsorbed bolometric flux of about 3x10-8 erg/cm2/s and a bolometric peak flux of 5x10-8 erg/cm2/s (errors < 20%). The latter provides an higher value for the distance estimation if compared with the one reported in Del Santo et al.

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