X-ray, UV, Optical and NIR Observations of Aql X-1

Details X-ray, UV, Optical and NIR Observations of Aql X-1 X-ray, UV, Optical and NIR Observations of Aql X-1

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2744....1m&link_type=abstract

The Astronomer's Telegram, #2744

Mathematics

Logic

1

Infra-Red, Optical, Ultra-Violet, X-Ray, Binaries, Neutron Stars, Transients

Scientific paper

Aql X-1 was observed using Swift between 2010 July 16.8965 and 2010 July 16.9083. The source was recently found to start a new outburst as inferred from Swift/BAT and MAXI/GSC monitoring data (ATEL #2742). Preliminary analyses of the XRT (WT mode) "quicklook" data suggests that the 0.6-10 keV spectrum can be well modeled (chi2/dof=565.2/400) by a phenomenological absorbed power law model with column density of (3.4 ± 0.02) E21 per cm2 and photon index 1.65 ± 0.05.

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