Supernova 1987A:30 years later - Cosmic Rays and Nuclei from Supernovae and their aftermaths
Contributed Papers
Progenitors of Core-Collapse Supernovae
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- 17 October 2017, pp. 1-10
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Evolution & Explosion of Massive Stars Leading to IIP-IIL SNe with MESA & SNEC
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- 17 October 2017, pp. 11-16
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Unveiling the structure of the progenitors of type-IIP Supernovae through multi-waveband observations
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- 17 October 2017, pp. 17-22
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Radio and X-ray observations of supernovae in dense environments
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- 17 October 2017, pp. 23-32
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Outbursts from evolved massive stars: SN 2015bh and its relatives
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- 17 October 2017, pp. 33-38
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The diversity of GRBs and their SNe: Observations from the 10.4m GTC
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- 17 October 2017, pp. 39-44
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Radioactive decay of GRB-SNe at late-times
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- 17 October 2017, pp. 45-50
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Properties of X-ray emission of an aspherical shock breakout
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- 17 October 2017, pp. 51-56
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Supernova 1986J: a Neutron Star or Black Hole in the Centre?
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- 17 October 2017, pp. 57-62
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Constraining pulsar birth properties with supernova X-ray observations
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- 17 October 2017, pp. 63-68
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Constraints on environs around SN 2011fe and SN 2014J from radio modeling and observations
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- 17 October 2017, pp. 69-74
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Spatial distribution of different subtypes of core-collapse and thermonuclear supernovae in the galaxies
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- 17 October 2017, pp. 75-80
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CSI in Supernova Remnants
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- 17 October 2017, pp. 81-85
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Diagnostics of the Supernova Engine
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- 17 October 2017, pp. 86-95
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Aspherical Supernovae and Oblique Shock Breakout
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- 17 October 2017, pp. 96-100
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Linking three-dimensional core-collapse supernova simulations with observations
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- 17 October 2017, pp. 101-106
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Core-Collapse Supernova Simulations including Neutrino Interactions from the Virial EOS
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- 17 October 2017, pp. 107-112
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Incidence of stellar rotation on the explosion mechanism of massive stars
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- 17 October 2017, pp. 113-118
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How to form a millisecond magnetar? Magnetic field amplification in protoneutron stars
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- 17 October 2017, pp. 119-124
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Magnetically assisted explosions of weakly magnetized stars
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- 17 October 2017, pp. 125-130
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