The end of the super-soft X-ray phase of the recurrent nova RS Ophiuchi

Details The end of the super-soft X-ray phase of the recurrent nova RS Ophiuchi The end of the super-soft X-ray phase of the recurrent nova RS Ophiuchi

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..838....1o&link_type=abstract

The Astronomer's Telegram, #838

Astronomy and Astrophysics

Astronomy

16

X-Ray, Novae

Scientific paper

Swift X-ray telescope observations of the recurrent nova RS Oph showed a linear decline in soft X-ray flux from a plateau level between Apr 12.1 and Apr 28.7 (ATEL #801). Since then Swift observations have continued, initially at nominal intervals of 2 days, and later, 4 days. The bright super-soft X-ray phase described in ATEL #770 (also CBET #498) appears to be over. The 0.3-10 keV count rate started to flatten out from its linear decline between the observations on May 10.6 and May 14.5.

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