Swift super soft X-ray detection in Nova V1213 Centauri

Details Swift super soft X-ray detection in Nova V1213 Centauri Swift super soft X-ray detection in Nova V1213 Centauri

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2904....1s&link_type=abstract

The Astronomer's Telegram, #2904

Astronomy and Astrophysics

Astronomy

1

Infra-Red, Optical, Ultra-Violet, X-Ray, Novae

Scientific paper

V1213 Cen was detected by Swift as a super soft X-ray source on March 26.9, 2010 with an average 0.3-10 keV count rate of 0.011 +/- 0.002 counts per second. V1213 Cen is a moderately fast classical nova with t_2 = 11 +/- 2 days based on the early AAVSO light curve. Additional Swift observations on April 27.1/28.5, July 20.3, August 17.7, and September 14.0, 2010 reveal that the source is becoming softer and brighter.

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