SN 2024qiw exhibits evidence of multiple major pre-explosion eruptions of clumpy circumstellar material at rates of at least 0.01 solar masses per year, implying LBV-like activity immediately before a Type II supernova.
Title resolution pending
4 Pith papers cite this work. Polarity classification is still indexing.
verdicts
UNVERDICTED 4representative citing papers
A new 3D dust reddening map with finer distance resolution, a spatial correlation prior, and Gaia-based distances covering the sky north of -30 degrees declination out to several kiloparsecs.
Close dual-AGN systems exhibit increased obscuration, higher bolometric luminosity, and elevated Eddington ratios for the less massive black hole as projected separation decreases, with excess AGN pairs relative to controls.
JH 223 shows a 250 G dipolar magnetic field truncating its disk near corotation, with accretion columns warping the inner disk to produce 3.31-day periodic dips in brightness.
citing papers explorer
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Giant outbursts of clumpy material preceding Type II supernova 2024qiw
SN 2024qiw exhibits evidence of multiple major pre-explosion eruptions of clumpy circumstellar material at rates of at least 0.01 solar masses per year, implying LBV-like activity immediately before a Type II supernova.
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A 3D Dust Map Based on Gaia, Pan-STARRS 1 and 2MASS
A new 3D dust reddening map with finer distance resolution, a spatial correlation prior, and Gaia-based distances covering the sky north of -30 degrees declination out to several kiloparsecs.
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Enhanced activity in close dual-AGN systems in the local Universe
Close dual-AGN systems exhibit increased obscuration, higher bolometric luminosity, and elevated Eddington ratios for the less massive black hole as projected separation decreases, with excess AGN pairs relative to controls.
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The circumstellar environment of the young, low-mass dipper star JH 223. Accretion and large-scale magnetic field topology
JH 223 shows a 250 G dipolar magnetic field truncating its disk near corotation, with accretion columns warping the inner disk to produce 3.31-day periodic dips in brightness.