Spectral evolution of galactic novae

Details Spectral evolution of galactic novae Spectral evolution of galactic novae

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..637..214m&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, Stellar Content And Populations, Morphology And Overall Structure

Scientific paper

We present low resolution spectroscopy of five galactic novae occurred in the years 1991 and 1992. Spectra spread over several months since outburst and show the spectroscopic evolution of the ejecta. We classify each nova according to the Cerro Tololo scheme. The spectroscopic classification is then considered in relation to the nova photometric evolution aiming to provide further evidence for a two nova populations in our Galaxy.

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