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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3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
representative citing papers
The maximum ejecta-to-accreted mass ratio in novae is at most ~2.6, set by nuclear energy release, contradicting claims of ratios up to 540 from orbital data.
ASASSN-16oh is interpreted as a non-ejective thermonuclear runaway on a 1.1 solar-mass white dwarf accreting at 3.5-5e-7 solar masses per year, with luminosity suppressed by an optically thick disk.
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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Upper bound of ejecta mass in a nova outburst
The maximum ejecta-to-accreted mass ratio in novae is at most ~2.6, set by nuclear energy release, contradicting claims of ratios up to 540 from orbital data.
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The supersoft X-ray transient ASASSN-16oh as a thermonuclear runaway without mass ejection
ASASSN-16oh is interpreted as a non-ejective thermonuclear runaway on a 1.1 solar-mass white dwarf accreting at 3.5-5e-7 solar masses per year, with luminosity suppressed by an optically thick disk.