X-ray spectroscopy of cataclysmic variables

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X-ray Spectroscopy of Cataclysmic Variables

In cataclysmic variables (CVs), accretion onto white dwarfs produces high temperature, high density plasmas. They cool down from kT∼10 keV via bremsstrahlung continuum and K and L shell line emissions. The small volume around white dwarfs means that the plasma densities are much higher than in, e.g., stellar coronae, probably beyond the range well-described by existing models. I will describe p...

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X-ray and Euv Spectroscopy of the Boundary Layer Emission of Nonmagnetic Cataclysmic Variables

EUVE , ROSAT , and ASCA observations of the boundary layer emission of nonmagnetic cataclysmic variables (CVs) are reviewed. EUVE spectra reveal that the effective temperature of the soft component of high-Ṁ nonmagnetic CVs is kT ∼ 10–20 eV and that its luminosity is∼ 0.1–0.5 times the accretion disk luminosity. Although the EUV spectra are very complex and belie simple interpretation, the phys...

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Two Types of X-ray Spectra in Cataclysmic Variables

We present Chandra HETG spectra of seven cataclysmic variables. We find that they divide unambiguously into two distinct types. Spectra of the first type are remarkably well fit by a simple cooling flow model, which assumes only steady-state isobaric radiative cooling. The maximum temperature, kTmax, and the normalization, which provides a highly precise measurement of the accretion rate, are t...

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The EUV and X-ray Emission of Nonmagnetic Cataclysmic Variables

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ژورنال

عنوان ژورنال: Advances in Space Research

سال: 2003

ISSN: 0273-1177

DOI: 10.1016/s0273-1177(03)90646-6