Spatially resolved spectroscopy shows SDSS1335+0728 has a three-zone ionisation structure, optically thin dust, and sustained low-level nuclear activity for at least 1500 years, implying the Ansky event is a faint transient in an already accreting low-mass SMBH.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Quantum hydrodynamic simulation of a helium white dwarf disrupted by a black hole predicts quantized vortices generating flickering EM radiation in the accretion disk and gravitational waves from the elongated white dwarf.
citing papers explorer
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Spatially resolved optical and mid-infrared spectroscopy of SDSS1335+0728: implications for the origin of the Ansky event
Spatially resolved spectroscopy shows SDSS1335+0728 has a three-zone ionisation structure, optically thin dust, and sustained low-level nuclear activity for at least 1500 years, implying the Ansky event is a faint transient in an already accreting low-mass SMBH.
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Searching for cosmic vortices
Quantum hydrodynamic simulation of a helium white dwarf disrupted by a black hole predicts quantized vortices generating flickering EM radiation in the accretion disk and gravitational waves from the elongated white dwarf.