Spectropolarimetry of SN 2026gzf indicates mostly spherical ejecta with axisymmetric Ca distribution viewed at ~40° from symmetry axis.
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3 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.HE 3representative citing papers
EP260321a is identified as the faintest shock breakout X-ray transient associated with broad-lined Ic supernova SN 2026gzf, interpreted as originating from a mildly relativistic weak outflow choked inside the progenitor star.
citing papers explorer
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Pinning Down the Geometry of the Type Ic Broad-Line Supernova 2026gzf
Spectropolarimetry of SN 2026gzf indicates mostly spherical ejecta with axisymmetric Ca distribution viewed at ~40° from symmetry axis.
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EP260321a/SN 2026gzf: The Faintest Shock Breakout Associated with a Broad-Lined Supernova
EP260321a is identified as the faintest shock breakout X-ray transient associated with broad-lined Ic supernova SN 2026gzf, interpreted as originating from a mildly relativistic weak outflow choked inside the progenitor star.