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Measuring White Dwarf Accretion Rates via Their Effective Temperatures

  • Townsley D
  • Bildsten L
The Astrophysical Journal (2003) 596(2) L227-L230
DOI: 10.1086/379535
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Abstract

Our previous theoretical study of the impact of an accreting envelope on the thermal state of an underlying white dwarf (WD) has yielded equilibrium core temperatures, classical nova ignition masses, and thermal lu-minosities for WDs accreting at time-averaged rates of. These values are 11 8 1

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Townsley, D. M., & Bildsten, L. (2003). Measuring White Dwarf Accretion Rates via Their Effective Temperatures. The Astrophysical Journal, 596(2), L227–L230. https://doi.org/10.1086/379535

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