Spectral and infrared differences between nova-links and dwarf novae

Details Spectral and infrared differences between nova-links and dwarf novae Spectral and infrared differences between nova-links and dwarf novae

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.236..259w&link_type=abstract

In ESA Recent Results on Cataclysmic Variables p 259-262 (SEE N86-20287 10-93)

Computer Science

7

Infrared Spectra, Line Spectra, Novae, Stellar Spectra, Accretion Disks, Cataclysmic Variables, Classifications, Photoionization, Stellar Color

Scientific paper

Differences between nova-like systems and dwarf nova are compared using the emission lines and infrared colors as a discriminant. The comparison using spectral lines clearly separates different classes of cataclysmic variables. Most nova-likes occupy the region near the line that describes the polars and intermediate polars indicating very similar ionization conditions. Several nova-likes are located within the dwarf novae region. Infrared data show that nova-likes tend to be redder than dwarf novae.

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