SN 2009ip at late times – an interacting transient at +2 years

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SN 2015bh: NGC 2770’s 4th supernova or a luminous blue variable on its way to a Wolf-Rayet star?LSQ13fn: A type II-Plateau supernova with a possibly low metallicity progenitor that breaks the standardised candle relation

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Q57578813-815BBAC3-85E0-41C1-ADF1-92649EE22EEA Q58059018-766A8A16-E417-4A13-AFFE-F67D7D5CE4C2

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SN 2009ip at late times – an interacting transient at +2 years

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http://www.wikidata.org/entity/Q58909418

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im September 2015 veröffentlichter wissenschaftlicher Artikel

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wetenschappelijk artikel

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наукова стаття, опублікована у вересні 2015

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SN 2009ip at late times – an interacting transient at +2 years

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SN 2009ip at late times – an interacting transient at +2 years

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SN 2009ip at late times – an interacting transient at +2 years

@en

SN 2009ip at late times – an interacting transient at +2 years

@nl

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SN 2009ip at late times – an interacting transient at +2 years

@en

SN 2009ip at late times – an interacting transient at +2 years

@nl

P1476

SN 2009ip at late times – an interacting transient at +2 years

@en

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Anders Jerkstrand

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

Andrea Pastorello

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

Antonia Morales-Garoffolo

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

Avishay Gal-Yam

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

Bonnie Zhang

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

Christopher Ashall

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

D. Andrew Howell

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

David R. Young

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

Emma S. Walker

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

Erkki Kankare

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

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Slowly fading super-luminous supernovae that are not pair-instability explosions

Fundamental properties of core-collapse supernova and GRB progenitors: predicting the look of massive stars before death

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

An outburst from a massive star 40 days before a supernova explosion.

A giant outburst two years before the core-collapse of a massive star.

An asymptotic-giant-branch star in the progenitor system of a type Ia supernova.

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

How Massive Single Stars End Their Life

The evolution of massive stars and their spectra. I. A non-rotating 60 M_{sun}_ star from the zero-age main sequence to the pre-supernova stage

Luminous blue variable eruptions and related transients: diversity of progenitors and outburst properties

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3886–3905

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

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scholarly article

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10.1093/MNRAS/STV1919

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

P407

English

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

P478

453

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

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P577

2015-09-14T00:00:00Z

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

P818

1502.06033

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

P819

2015MNRAS.453.3886F

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

SN 2009ip at late times – an interacting transient at +2 years

about

P2860

P2860

SN 2009ip at late times – an interacting transient at +2 years

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