X-ray spectral modeling and timing analysis of V1674 Her constrain its white dwarf mass to 1.09-1.12 solar masses, well below the near-Chandrasekhar value expected from its t2~1 day decline time.
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VLA observations of six cataclysmic variables reveal polarized radio emission consistent with coherent mechanisms like electron-cyclotron maser emission or plasma radiation.
citing papers explorer
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X-ray spectroscopy mass constraints on V1674 Her: the fastest nova does not have a near-Chandrasekhar white dwarf
X-ray spectral modeling and timing analysis of V1674 Her constrain its white dwarf mass to 1.09-1.12 solar masses, well below the near-Chandrasekhar value expected from its t2~1 day decline time.
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A broadband search for coherent radio emission in cataclysmic variables
VLA observations of six cataclysmic variables reveal polarized radio emission consistent with coherent mechanisms like electron-cyclotron maser emission or plasma radiation.