An Extended Grid of Nova Models. II. The Parameter Space of Nova Outbursts
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- 10 April 2005
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 623 (1), 398-410
- https://doi.org/10.1086/428435
Abstract
This paper is a sequel to an earlier paper devoted to multiple, multicycle nova evolution models (Prialnik & Kovetz, Paper I), which showed that the different characteristics of nova outbursts can be reproduced by varying the values of three basic and independent parameters: the white dwarf mass, MWD, the temperature of its isothermal core, TWD, and the mass transfer rate, . Here we show that the parameter space is constrained by several analytical considerations and find its limiting surfaces. Consequently, we extend the grid of multicycle nova evolution models presented in Paper I to its limits, adding multicycle nova outburst calculations for a considerable number of new parameter combinations. In particular, the extended parameter space that produces nova eruptions includes low mass transfer rates down to 5 × 10-13 M☉ yr-1 and more models for low TWD. Resulting characteristics of these runs are added to the former parameter combination results to provide a full grid spanning the entire parameter space for carbon-oxygen white dwarfs. The full grid covers the entire range of observed nova characteristics, even those of peculiar objects, which have not been numerically reproduced until now. Most remarkably, runs for very low lead to very high values for some characteristics, such as outburst amplitude A 20, high super-Eddington luminosities at maximum, heavy element abundance of the ejecta Zej ≈ 0.63, and high ejected masses mej ≈ 7 × 10-4 M☉.Keywords
This publication has 24 references indexed in Scilit:
- On the Properties of Galactic Novae and Their Orbital Period DistributionThe Astrophysical Journal, 2004
- White Dwarf Sequences in Dense Star ClustersThe Astrophysical Journal, 2003
- The effect of heating from the boundary layer on accretion models for novae and other compact objectsThe Astrophysical Journal, 1987
- Stellar accretion of matter possessing angular momentumThe Astrophysical Journal, 1987
- CNO abundances resulting from diffusion in accreting nova progenitorsThe Astrophysical Journal, 1985
- CNO abundances and the strengths of nova outbursts and hydrogen flashes on accreting white dwarfsThe Astrophysical Journal, 1983
- A theory of hydrogen shell flashes on accreting white dwarfs. I - Their progress and the expansion of the envelope. II - The stable shell burning and the recurrence period of shell flashesThe Astrophysical Journal, 1982
- What determines the speed class of novaeThe Astrophysical Journal, 1980
- A single-star interpretation of Nova Cygni 1975The Astrophysical Journal, 1976
- Analytic Approximations to the Mass-Radius Relation and Energy of Zero-Temperature StarsThe Astrophysical Journal, 1972