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2013

Evolution of accreting white dwarfs; some of them continue to grow

Newsham, G., Starrfield, S., Timmes, F.

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Novae are cataclysmic variable binary systems in which a white dwarf primary is accreting material from a low mass companion.

The importance of this accretion takes on added significance if the WD can increase its mass to reach the Chandrasekhar limit thus exploding as a Type Ia supernova.
In this study we accrete material of Solar composition onto carbon-oxygen white dwarfs of 0.70, 1.00 and 1.35 Msun with accretion rates from 1.6e-10 to 1.6e-6 Msun per yr.
We have utilized the MESA stellar evolution code for our modeling and evolve them for many nova cycles or, in some cases, evolution to a red giant stage.

Evolution of accreting white dwarfs; some of them continue to grow · Around

Built on

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Starrfield, S., Timmes, F. X., Iliadis, C., Hix, W. R., Arnett, W. D., Meakin, C., & Sparks, W. M. 2012b, Baltic Astronomy, 21, 76
Original
Cited in the paper.

Then

Paxton, B., Bildsten, L., Dotter, A., Herwig, F., Lessafre, P., & Timmes, F. 2011, ApJS, 192, 3
2011
Later among the works it cites.
Idan, I., Shaviv, N. J., & Shaviv, G. 2012, Journal of Physics: Conference Series, 337, 012051
2012
Later among the works it cites.
Denissenkov, P. A., Herwig, F., Bildsten, L., & Paxton, B. 2013, ApJ, 762, 8
2013
Closest in time.
Paxton, B., Cantiello, P., M. Arras, Bildsten, L., Brown, E., Dotter, A., Mankovich, C., Montgomery, D., M. Stello, Timmes, F., & Townsend, R. 2013, astro-ph. 1301.0319
2013
Closest in time.

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