The early outburst light curve of the 2011 eruption of the Recurrent Nova T Pyxidis from Solar Mass Ejection Imager (SMEI) observations

Details The early outburst light curve of the 2011 eruption of the Recurrent Nova T Pyxidis from Solar Mass Ejection Imager (SMEI) observations The early outburst light curve of the 2011 eruption of the Recurrent Nova T Pyxidis from Solar Mass Ejection Imager (SMEI) observations

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3373....1h&link_type=abstract

The Astronomer's Telegram, #3373

Astronomy and Astrophysics

Astronomy

Optical, Nova

Scientific paper

We report white light observations of the 2011 outburst of Recurrent Nova T Pyxidis obtained using the USAF/NASA Solar Mass Ejection Imager (SMEI) on board the Coriolis satellite (see Hounsell et al., 2010 for details, all magnitudes quoted here are native to the SMEI photometric system). The instrument has a peak quantum efficiency at approximately 700 nm with a FWHM ~ 300 nm.

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