Circumstellar Light Echo as a Possible Origin of the Polarization of Type IIP Supernovae
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/847/i=2/a=111/pdf
Reference73 articles.
1. CHARACTERIZING THEV-BAND LIGHT-CURVES OF HYDROGEN-RICH TYPE II SUPERNOVAE
2. EVIDENCE FOR PRE-EXISTING DUST IN THE BRIGHT TYPE IIn SN 2010jl
3. Detection of a Massive Dust Shell around the Type II Supernova SN 2002hh
4. BOLOMETRIC LIGHT CURVES FOR 33 TYPE II PLATEAU SUPERNOVAE
5. AXISYMMETRIC AB INITIO CORE-COLLAPSE SUPERNOVA SIMULATIONS OF 12-25 M ☉ STARS
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1. Diversity of Dust Properties in External Galaxies Confirmed by Polarization Signals from Type II Supernovae;The Astrophysical Journal Letters;2022-12-01
2. The Effects of Circumstellar Dust Scattering on the Light Curves and Polarizations of Type Ia Supernovae*;The Astrophysical Journal;2022-06-01
3. PGIR 20eid (SN 2020qmp): A Type IIP Supernova at 15.6 Mpc discovered by the Palomar Gattini-IR survey;Astronomy & Astrophysics;2022-04
4. Infrared spectropolarimetric detection of intrinsic polarization from a core-collapse supernova;Nature Astronomy;2021-03-11
5. The aspherical explosion of the Type IIP SN 2017gmr†;Monthly Notices of the Royal Astronomical Society: Letters;2019-09-05
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