Computer Science
Scientific paper
Jun 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.236..229d&link_type=abstract
In ESA Recent Results on Cataclysmic Variables p 229-232 (SEE N86-20287 10-93)
Computer Science
2
Cataclysmic Variables, Explosions, Magnesium, Neon, Novae, Stellar Composition, White Dwarf Stars, Nuclear Fusion, Stellar Evolution, Stellar Mass Accretion, Stellar Temperature
Scientific paper
Nova explosions in cataclysmic variables containing an oxygen neon magnesium white dwarf are considered. It is shown that these systems might contribute to a non negligible fraction of the observed classical nova outbursts. Using a simple model, the time evolution of bolometric luminosity, effective temperature, and temperature and density at the bottom of the accreted layer during one outburst are calculated. The consequences of shear mixing between the accreted layer and the white dwarf material are investigated in relation with observations of 2 neon enriched novae (Nova V 693 CrA 1981 and Nova Aql 1982). Nucleosynthesis in such objects is discussed.
Delbourgo-Salvador Pascale
Mochkovitch Robert
Vangioni-Flam Elisabeth
No associations
LandOfFree
Nova explosion on oxygen neon magnesium white dwarfs does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Nova explosion on oxygen neon magnesium white dwarfs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nova explosion on oxygen neon magnesium white dwarfs will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1667630