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Related papers: Three-Dimensional Explosion Geometry of Stripped-E…

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We present modelling of line polarization to study multi-dimensional geometry of stripped-envelope core-collapse supernovae (SNe). We demonstrate that a purely axisymmetric, two-dimensional geometry cannot reproduce a loop in the Stokes Q-U…

High Energy Astrophysical Phenomena · Physics 2017-03-15 Masaomi Tanaka , Keiichi Maeda , Paolo A. Mazzali , Koji S. Kawabata , Ken'ichi Nomoto

We briefly review the existing database of supernova spectropolarimetry, concentrating on recent data and on results from our group's research. Spectropolarimetry provides the only direct known probe of early-time supernova geometry. To…

Astrophysics · Physics 2007-05-23 Alexei V. Filippenko , Douglas C. Leonard

An important and perhaps critical clue to the mechanism driving the explosion of massive stars as supernovae is provided by the accumulating evidence for asymmetry in the explosion. Indirect evidence comes from high pulsar velocities,…

Polarization has been detected at early times for all types of supernova, indicating that such systems result from or quickly develop some form of asymmetry. In addition, the detection of strong line polarization in supernovae is suggestive…

High Energy Astrophysical Phenomena · Physics 2015-05-19 K. T. Hole , D. Kasen , K. H. Nordsieck

We discuss the optical spectropolarimetry of several core-collapse supernovae, SN 1996cb (Type IIB), SN 1997X (Type Ic), and SN 1998S (Type IIn). The data show polarization evolution of several spectral features at levels from 0.5% to above…

Astrophysics · Physics 2007-05-23 Lifan Wang , D. Andrew Howell , Peter Hoeflich , J. Craig Wheeler

Overwhelming evidence has accumulated in recent years that supernova explosions are intrinsically 3-dimensional phenomena with significant departures from spherical symmetry. We review the evidence derived from spectropolarimetry that has…

Astrophysics · Physics 2008-12-18 Lifan Wang , J. Craig Wheeler

The explosion processes of supernovae (SNe) are imprinted in their explosion geometries. Here, we study the intrinsic polarization of 15 hydrogen-rich core-collapse SNe and explore the relation with the photometric and spectroscopic…

High Energy Astrophysical Phenomena · Physics 2024-01-10 T. Nagao , F. Patat , A. Cikota , D. Baade , S. Mattila , R. Kotak , H. Kuncarayakti , M. Bulla , B. Ayala

We present six epochs of spectropolarimetric observations and one epoch of spectroscopy of the Type Ib SN iPTF 13bvn. The epochs of these observations correspond to $-$10 to $+$61 days with respect to the {\it r}-band light curve maximum.…

The measurement of non-zero polarization can be used to infer the presence of departures from spherical symmetry in supernovae (SNe). The origin of the majority of the intrinsic polarization observed in SNe is in electron scattering, which…

Solar and Stellar Astrophysics · Physics 2023-09-01 J. R. Maund

We present 645 optical spectra of 73 supernovae (SNe) of Types IIb, Ib, Ic, and broad-lined Ic. All of these types are attributed to the core collapse of massive stars, with varying degrees of intact H and He envelopes before explosion. The…

Recent observations of core-collapse supernovae (SNe) suggest aspherical explosions. Globally aspherical structures in SN explosions are regarded as the key for understanding their explosion mechanism. However, the exact explosion…

We present single-epoch, post-maximum spectropolarimetry of four Type Ia supernovae (SNe Ia) that span a range of spectral and photometric properties: SN 2002bf and SN 2004dt exhibit unusually high-velocity (HV) absorption lines. SN 1997dt…

Over the past 30 years, spectropolarimetry has proven to be a great tool to probe the 3D geometry of core collapse supernovae (CCSNe). The number of high-quality multi-epoch spectropolarimetric data sets for CCSNe remains quite low,…

Solar and Stellar Astrophysics · Physics 2019-06-19 H. F. Stevance

We present an analysis of the nebular spectra of 103 stripped envelope (SE) supernovae (SNe) collected from the literature and observed with the Subaru Telescope from 2002 to 2012, focusing on [O I] 6300, 6363. The line profile and width of…

We present the first spectropolarimetric observations of a hydrogen-free superluminous supernova at z=0.1136, namely SN 2015bn. The transient shows significant polarization at both the observed epochs: one 24 days before maximum light in…

High Energy Astrophysical Phenomena · Physics 2016-11-09 C. Inserra , M. Bulla , S. A. Sim , S. J. Smartt

SN 1993J is one of the best studied Type IIb supernovae. Spectropolarimetric data analyses were published over two decades ago at a time when the field of supernova spectropolarimetry was in its infancy. Here we present a new analysis of…

Solar and Stellar Astrophysics · Physics 2020-04-01 H. F. Stevance , D. Baade , J. R. Bruten , A. Cikota , A. Clocchiatti , D. C. Hines , P. Höflich , J. R. Maund , F. Patat , P. J. Vallely , J. C. Wheeler

I present an overview of optical observations (mostly spectra) of Type II, Ib, and Ic supernovae (SNe). SNe II are defined by the presence of hydrogen, and exhibit a very wide variety of properties. SNe II-L tend to show evidence of…

Astrophysics · Physics 2009-11-06 Alexei V. Filippenko

We investigate polarization spectra of hydrogen-rich core-collapse supernovae (Type~II SNe). The polarization signal from SNe contains two independent components: intrinsic SN polarization and interstellar polarization (ISP). From these…

Astrophysics of Galaxies · Physics 2023-10-04 T. Nagao , S. Mattila , R. Kotak , H. Kuncarayakti

We present observations and analysis of 18 stripped-envelope supernovae observed during 2013 -- 2018. This sample consists of 5 H/He-rich SNe, 6 H-poor/He-rich SNe, 3 narrow lined SNe Ic and 4 broad lined SNe Ic. The peak luminosity and…

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