Swift detects a large flux increase and a probable period of 1.77 days in the X-ray and UV emission of the nova CSS081007:030559+054715

Details Swift detects a large flux increase and a probable period of 1.77 days in the X-ray and UV emission of the nova CSS081007:030559+054715 Swift detects a large flux increase and a probable period of 1.77 days in the X-ray and UV emission of the nova CSS081007:030559+054715

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1873....1b&link_type=abstract

The Astronomer's Telegram, #1873

Astronomy and Astrophysics

Astronomy

8

Ultra-Violet, X-Ray, Request For Observations, Novae

Scientific paper

Swift has continued to monitor the nova CSS081007:030559+054715 (ATEL #1825, ATEL #1835, ATEL #1847) in the X-ray and UV wavebands. The Swift-XRT 0.3-10 keV light curve showed a relatively constant count rate of 0.18-0.21 count/s from 2008-Nov-10 to 2008-Nov-21. Over the same time interval the Swift-UVOT uvw2 light curve (central wavelength 1928 A) had a mean magnitude of 14.9, with +/-0.2 magnitude deviations from this value.

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