Amanote Research

Amanote Research

    RegisterSign In

GRB 130603B: No Compelling Evidence for Neutron Star Merger

Advances in Astronomy - United States
doi 10.1155/2015/460293
Full Text
Open PDF
Abstract

Available in full text

Categories
AstrophysicsAstronomyPlanetary ScienceSpace
Date

January 1, 2015

Authors
Shlomo DadoArnon Dar
Publisher

Hindawi Limited


Related search

Electromagnetic Evidence That SSS17a Is the Result of a Binary Neutron Star Merger

Science
MultidisciplinaryPhilosophy of ScienceHistory
2017English

Multi-Messenger Observations of a Binary Neutron Star Merger

2019English

R-Process Nucleosynthesis in a Double Neutron-Star Merger: The Case of GW170817

2019English

Neutron Star Merger Remnants: Braking Indices, Gravitational Waves, and the Equation of State

2019English

Detectability of Gravitational Wave Bursts From a Class of Neutron Star Starquake GRB Models

International Journal of Modern Physics D
AstrophysicsAstronomyPlanetary ScienceMathematical PhysicsSpace
1996English

Evidence-Based Search Method for Gravitational Waves From Neutron Star Ring-Downs

Physical Review D
2007English

A Unified Binary Neutron Star Merger Magnetar Model for the Chandra X-Ray Transients CDF-S XT1 and XT2

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

Bayes Factor Design Analysis: Planning for Compelling Evidence

SSRN Electronic Journal
2016English

Neutron Star Atmospheres

International Astronomical Union Colloquium
2000English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy