XMM-Newton and Swift-XRT see declining X-ray flux from the nova XMMSL1 J070542.7-381442 (V598 Pup)

Details XMM-Newton and Swift-XRT see declining X-ray flux from the nova XMMSL1 J070542.7-381442 (V598 Pup) XMM-Newton and Swift-XRT see declining X-ray flux from the nova XMMSL1 J070542.7-381442 (V598 Pup)

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1301....1r&link_type=abstract

The Astronomer's Telegram, #1301

Astronomy and Astrophysics

Astronomy

5

Novae, Transients

Scientific paper

The bright new X-ray transient, XMMSL1 J070542.7-381442 (= V598 Pup [IAUC #8898]), discovered by ESA's XMM-Newton in its Slew Survey mode [ATel #1282] and identified as a classical nova [ATel #1285], has been observed by XMM-Newton in its normal pointed mode and by Swift. The observed 0.2-2 keV EPIC-pn count rate has declined from 53.7 ct/s (XMM-Slew, rev.1434, obsid 9143400002, full-frame, medium filter: 2007-10-08 [ATel #1282]) to 3.7 ct/s (XMM-pointed, rev.1445, obsid 0510010901, 5 ksec exposure, small window, medium filter, 2007-10-30).

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