Are Swift gamma-ray bursts consistent with the Ghirlanda relation? - Wikidata - wikimedia - TriplyDB

Are Swift gamma-ray bursts consistent with the Ghirlanda relation?

Are Swift gamma-ray bursts consistent with the Ghirlanda relation?

http://www.wikidata.org/entity/Q58913381

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Diversity of gamma-ray burst energetics vs. supernova homogeneity: SN 2013cq associated with GRB 130427A Suzaku Wide-band All-sky Monitor (WAM) observations of GRBs and SGRs

P2860

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Are Swift gamma-ray bursts consistent with the Ghirlanda relation?

http://www.wikidata.org/entity/Q58913381

description

article publié dans la revue scientifique Astronomy and Astrophysics

@fr

im April 2007 veröffentlichter wissenschaftlicher Artikel

@de

scientific article published in Astronomy and Astrophysics

@en

wetenschappelijk artikel

@nl

наукова стаття, опублікована у квітні 2007

@uk

name

Are Swift gamma-ray bursts consistent with the Ghirlanda relation?

@en

Are Swift gamma-ray bursts consistent with the Ghirlanda relation?

@nl

type

label

Are Swift gamma-ray bursts consistent with the Ghirlanda relation?

@en

Are Swift gamma-ray bursts consistent with the Ghirlanda relation?

@nl

prefLabel

Are Swift gamma-ray bursts consistent with the Ghirlanda relation?

@en

Are Swift gamma-ray bursts consistent with the Ghirlanda relation?

@nl

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0004-6361:20066984

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Astronomy and Astrophysics

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Are Swift gamma-ray bursts consistent with the Ghirlanda relation?

@en

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A. Moretti

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

C. Guidorzi

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

D. Rizzuto

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

G. Chincarini

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

S. Campana

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

P2860

No supernovae associated with two long-duration gamma-ray bursts

A novel explosive process is required for the gamma-ray burst GRB 060614.

The Supernova–Gamma-Ray Burst Connection

Jets in Gamma-Ray Bursts

Evidence for a Canonical Gamma‐Ray Burst Afterglow Light Curve in theSwiftXRT Data

Measurements of Ω and Λ from 42 High‐Redshift Supernovae

A Spectacular Radio Flare from XRF 050416a at 40 Days and Implications for the Nature of X‐Ray Flashes

Multiwavelength Observations of GRB 050820A: An Exceptionally Energetic Event Followed from Start to Finish

Gamma-Ray Burst Afterglows

The Dynamics and Light Curves of Beamed Gamma‐Ray Burst Afterglows

P304

395–401

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scholarly article

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10.1051/0004-6361:20066984

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P407

P433

2

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472

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Gianpiero Tagliaferri

Patrizia Romano

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2007-04-24T00:00:00Z

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astro-ph/0703676

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P819

2007A&A...472..395C

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