An aspherical distribution for the explosive burning ash of core-collapse supernovae
- 26 October 2023
- journal article
- research article
- Published by Springer Nature in Nature Astronomy
- Vol. 8 (1) , 111-118
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- The Unique Type Ib Supernova 2005bf at Nebular Phases: A Possible Birth Event of a Strongly Magnetized Neutron StarThe Astrophysical Journal, 2007
- SN 2006aj Associated with XRF 060218 at Late Phases: Nucleosynthesis Signature of a Neutron Star-driven ExplosionThe Astrophysical Journal, 2007
- An optical supernova associated with the X-ray flash XRF 060218Nature, 2006
- An Asymmetric Energetic Type Ic Supernova Viewed Off-Axis, and a Link to Gamma Ray BurstsScience, 2005
- Evolution, Explosion, and Nucleosynthesis of Core‐Collapse SupernovaeThe Astrophysical Journal, 2003
- Stability of Standing Accretion Shocks, with an Eye toward Core‐Collapse SupernovaeThe Astrophysical Journal, 2003
- The evolution and explosion of massive starsReviews of Modern Physics, 2002
- Bipolar Supernova ExplosionsThe Astrophysical Journal, 2001
- Jet-induced Explosions of Core Collapse SupernovaeThe Astrophysical Journal, 1999
- The evolution and explosion of massive binary stars and Type Ib-Ic-IIb-IIL supernovaePhysics Reports, 1995