Classical Nova Evolution: Clues from Soft X-ray Emission
作者： James Macdonald
DOI: 10.1007/978-94-009-0325-8_82
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摘要: Multi-wavelength observations have shown that, after optical decline, the stellar remnants of classical nova outbursts evolve at constant, near-Eddington, bolometric luminosity to high effective temperature (> 2105 K), before turning off. Here we briefly review novae in this phase evolution, and discuss what soft X-ray tell us about mass underlying white dwarf rate change due winds accretion from companion.
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