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Stellar collision
Black-Hole Binaries, Gravitational Waves, and Numerical Relativity
Are Gamma-Ray Bursts Signals of Supermassive Black Hole Formation?
Gamma Ray Bursts from Stellar Collisions
The Time of Perihelion Passage and the Longitude of Perihelion of Nemesis
Colliding Stars Spark Rush to Solve Cosmic Mysteries Stellar Collision Confirms Theoretical Predictions About the Periodic Table
Gamma Ray Bursts from Stellar Collisions
Frederic A. Rasio — Publication List
Instituto De Astrofísica De Andalucía IAA-CSIC
Evolution of Stellar Collision Products in Globular Clusters – I
Survivor of Stellar Collision Is New Type of Pulsating Star 28 June 2013
Formation of Supermassive Black Holes in the Early Universe
Survivability of Planetary Systems in Young and Dense Star Clusters the Free-floating Stars in the Cluster
SCIENTIFIC OSJECTIVES of DEEP SPACE INVESTIGATIONS : the ORIGIN and EVOLUTION of the SOLLAR SYSTEM * Report P-18
Galaxy Collide
Nuclear Detonation Around Compact Objects
Uva-DARE (Digital Academic Repository)
The Globular Cluster Mass/Low Mass X-Ray Binary Correlation: Implications for Kick Velocity Distributions from Supernovae
1. Introduction
Top View
The Evolution of Runaway Stellar Collision Products
Arxiv:1612.04395V3 [Astro-Ph.SR] 12 Jul 2017 1 University of Virginia, Charlottesville, VA 22904, USA Holes (Freire Et Al
Exploring Intermediate and Massive Black-Hole Binaries with the Einstein Telescope
EASTER 2018 Widden Whinnies Inglis Easter Crackers
9 Feb 2010 Young Massive Star Clusters
The Evolution of Runaway Stellar Collision Products
X-Ray Searches for Axions from Super Star Clusters
The Extragalactic Perspective
NL9 CH12 2Nd B.Indd
Stellar Collision Triggers Supernova Explosion 2 September 2021
Stellar and Gas Dynamics in Galactic Nuclei
Properties of Unusually Luminous Supernovae
Submillimeter Array Newsletter Number 29, January 2020 CONTENTS from the DIRECTOR
The Secret Lives of Stars 2004
By David J. Eicher
Modelling the Stellar Soft-Photon Energy Density Profile of Globular
Survivability of Planetary Systems in Young and Dense Star Clusters A
Exploring Intermediate and Massive Black-Hole Binaries with the Einstein Telescope
The Effects of Stellar Collisions in Dense Environments
19 66Apj. . .143. .400S on the EVOLUTION of GALACTIC
Arxiv:1807.06593V1 [Astro-Ph.GA] 17 Jul 2018
Supernovae Represent a Catastrophic Phenomenon of Far Greater Magni- Tude and Much Smaller Frequency Than Do Ordinary Novae
On the Onset of Runaway Stellar Collisions in Dense Star Clusters - I
Gravitational-Wave Astronomy
Type Ia Supernova
Supernovae. Part I: the Events
Unit 1 Space Suggested Time: 21 Hours SPACE
Young Massive Star Clusters
Supernovae Represent a Catastrophic Phenomenon of Far Greater Magni- Tude and Much Smaller Frequency Than Do Ordinary Novae
We Are Not Star Dust . on Collision of Neutron Stars , Production of Heavy
Transactions 1904
Chapter 12 Space Exploration Section 12.1 Page 428 Explaining the Early Universe
Energetic Explosions from Collisions of Stars at Relativistic Speeds in Galactic Nuclei