Detection of a micronova burst in TESS data of IGR J17014-4306, with inferred burned mass 1.6e-11 solar masses and recurrence time ~20 days, adding the eighth confirmed system.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.HE 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Chandra HETG spectroscopy of BZ Cam diagnoses an ADAF-like advective hot flow with plasma densities of a few times 10^12-14 cm^-3, temperatures of 3-30 million K, and nonequilibrium ionization conditions.
citing papers explorer
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A micronova burst in the intermediate polar IGR J17014-4306
Detection of a micronova burst in TESS data of IGR J17014-4306, with inferred burned mass 1.6e-11 solar masses and recurrence time ~20 days, adding the eighth confirmed system.
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High Resolution X-ray Spectroscopy of the Nova-Like Cataclysmic Variable BZ Cam using Chandra HETG: Diagnosis of the ADAF-like (Advective) Hot Flow
Chandra HETG spectroscopy of BZ Cam diagnoses an ADAF-like advective hot flow with plasma densities of a few times 10^12-14 cm^-3, temperatures of 3-30 million K, and nonequilibrium ionization conditions.