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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2 Pith papers cite this work. Polarity classification is still indexing.
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Advocates for a 2deg x 0.4deg multi-wavelength SKA-Mid continuum survey plus decade-long monitoring of the Galactic Centre nuclear star cluster to address multiple science questions with one dataset.
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 Nearest Galactic Nucleus: Studying the Galactic Centre with SKA-Mid
Advocates for a 2deg x 0.4deg multi-wavelength SKA-Mid continuum survey plus decade-long monitoring of the Galactic Centre nuclear star cluster to address multiple science questions with one dataset.