Long-term X-ray monitoring indicates Swift J174610.4-290018 is a recurrent nova similar to RS Oph rather than an accretion-disk corona source.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
representative citing papers
SED modeling of early 2021 RS Oph data indicates bipolar ejecta with equatorial disk and confirms significant WD radiation originates from reprocessed shock emission explained by WD rotation.
SKAO will enable regular multi-frequency radio monitoring of Galactic novae to probe ionised and relativistic particle populations in classical and symbiotic systems.
citing papers explorer
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Is the Peculiar Galactic Center Transient Swift J174610.4-290018 A Nova Outburst?
Long-term X-ray monitoring indicates Swift J174610.4-290018 is a recurrent nova similar to RS Oph rather than an accretion-disk corona source.
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The first hours and days of the 2021 explosion of the recurrent symbiotic nova RS Ophiuchii
SED modeling of early 2021 RS Oph data indicates bipolar ejecta with equatorial disk and confirms significant WD radiation originates from reprocessed shock emission explained by WD rotation.
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Probing Physical Conditions in Classical and Symbiotic Novae with the Square Kilometre Array Observatory
SKAO will enable regular multi-frequency radio monitoring of Galactic novae to probe ionised and relativistic particle populations in classical and symbiotic systems.