IM Normae and N Sgr 2002: CCD Spectroscopy and Photometry

Details IM Normae and N Sgr 2002: CCD Spectroscopy and Photometry IM Normae and N Sgr 2002: CCD Spectroscopy and Photometry

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..637..289l&link_type=abstract

CLASSICAL NOVA EXPLOSIONS: International Conference on Classical Nova Explosions. AIP Conference Proceedings, Volume 637, pp. 2

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Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, Charge-Coupled Devices, Image Detectors, And Ir Detector Arrays, Photometric, Polarimetric, And Spectroscopic Instrumentation

Scientific paper

CCD photometry and spectrometry were carried out during the outbursts of the recurrent nova IM Normae and Nova Sagittarii 2002 = V4741 Sgr. The former in its first eruption since 1920 is, together with T Pyx, a second example of a slow recurrent nova. IM Nor started as a typical ``Fe II'' class nova, but after about two months, changed to a ``He/N'' nova (Williams [1]). N Sgr 2002 was discovered shortly before this conference began, and the results of only three nights are included. All the observations are presented and discussed in detail.

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