An analytic bolometric light curve model of interaction-powered supernovae and its application to Type IIn supernovae

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Interacting supernovae from photoionization-confined shells around red supergiant stars.Mass-loss histories of Type IIn supernova progenitors within decades before their explosion SN 2009ip at late times – an interacting transient at +2 years

P2860

Q50462722-299DB711-3BE7-4663-809E-5AAB5B389B5F Q58059186-8A6421C6-49B1-4667-93B0-17C462CBA0FE Q58909418-48DC661B-8E42-47D9-A7EB-8BDE3C0F42B8

P2860

An analytic bolometric light curve model of interaction-powered supernovae and its application to Type IIn supernovae

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http://www.wikidata.org/entity/Q58059228

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article

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im August 2013 veröffentlichter wissenschaftlicher Artikel

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wetenschappelijk artikel

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наукова стаття, опублікована в серпні 2013

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An analytic bolometric light c ...... ication to Type IIn supernovae

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An analytic bolometric light c ...... ication to Type IIn supernovae

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An analytic bolometric light c ...... ication to Type IIn supernovae

@en

An analytic bolometric light c ...... ication to Type IIn supernovae

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An analytic bolometric light c ...... ication to Type IIn supernovae

@en

An analytic bolometric light c ...... ication to Type IIn supernovae

@nl

P1476

An analytic bolometric light c ...... ication to Type IIn supernovae

@en

P2093

Elena I. Sorokina

http://www.w3.org/2001/XMLSchema#string

Keiichi Maeda

http://www.w3.org/2001/XMLSchema#string

Sergei I. Blinnikov

http://www.w3.org/2001/XMLSchema#string

Takashi J. Moriya

http://www.w3.org/2001/XMLSchema#string

P2860

Superluminous supernovae at redshifts of 2.05 and 3.90

Theoretical light curves for deflagration models of type Ia supernova

The mass-loss rates of red supergiants and the de Jager prescription

Caltech Core-Collapse Project (CCCP) observations of type IIn supernovae: typical properties and implications for their progenitor stars

Massive star evolution: luminous blue variables as unexpected supernova progenitors

A massive hypergiant star as the progenitor of the supernova SN 2005gl.

Type IIn supernovae at redshift z approximately 2 from archival data.

Pulsational pair instability as an explanation for the most luminous supernovae.

How Massive Single Stars End Their Life

On luminous blue variables as the progenitors of core-collapse supernovae, especially Type IIn supernovae

P304

1520–1535

http://www.w3.org/2001/XMLSchema#string

P31

scholarly article

P356

10.1093/MNRAS/STT1392

http://www.w3.org/2001/XMLSchema#string

P407

English

P433

http://www.w3.org/2001/XMLSchema#string

P478

435

http://www.w3.org/2001/XMLSchema#string

P50

Jesper Sollerman

Francesco Taddia

P577

2013-08-20T00:00:00Z

http://www.w3.org/2001/XMLSchema#dateTime

P818

1307.2644

http://www.w3.org/2001/XMLSchema#string

P819

2013MNRAS.435.1520M

http://www.w3.org/2001/XMLSchema#string

An analytic bolometric light curve model of interaction-powered supernovae and its application to Type IIn supernovae

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P2860

P2860

An analytic bolometric light curve model of interaction-powered supernovae and its application to Type IIn supernovae

description

name

type

label

prefLabel

P1433

P1476

P2093

P2860

P304

P31

P356

P407

P433

P478

P50

P577

P818

P819

P356

P1433

P1476

P2093

P2860

P304

P31

P356

P407

P433

P478

P50

P577

P818

P819