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Q star
1 Kepler's Third
Abbreviated Curriculum Vitae
Observations and Properties of Candidate High Frequency GPS
Introduzione Alla Cosmologia Fisica Lezione 14
Department of Physics Stanford University, Stanford, California 94305
Astrophysical Evidence for the Existence of Black Holes 3 Dissipated, Chandrasekhar Was Awarded a Share in the Nobel Prize for This Discovery
Black Hole Physics Entering a New Observational Era
Drops of Strange Chiral Nucleon Liquid (SNL) & Ordinary Chiral Heavy Nuclear Liquid (NL)
Astronomy 114 – Summary of Important Concepts #2 1 Stars: Key
Neil Degrasse Tyson, Answers Our Questions About the 'Cosmos
Investigating High Field Gravity Using Astrophysical Techniques
Appendix a TABLES of Eoss in NEUTRON STAR CRUST
A Numerical Study of Solitonic Boson Stars in General Relativity
Are Q-Stars a Serious Threat for Stellar-Mass Black Hole Candidates?
“Neutron” Stars?
Physical Processes in the Interstellar Medium
Superfluid Hydrodynamics in Neutron Stars By
Black Hole Physics: Recent Developments and Observational Perspectives
Top View
An Upper Bound on Q-Star Masses Onic Matter Is Particularly Interesting Because It Offers a Consistent Description Of
Arxiv:2105.02116V1 [Physics.Gen-Ph] 5 Jan 2021 Rbesses[] Unu Rusadqatmal- Quantum and Groups Inte- As Quantum Quantum Such of Gebras, Theory [1]
Surveying Stars
INTEGRAL Upper Limits on Gamma-Ray Emission Associated with the Gravitational Wave Event GW150914
The Impact of Photoionization on Star Formation at Molecular Cloud Scales
No Observational Proof of the Black-Hole Event-Horizon
Gravity and Black Hole Astronomy Connections
Author Index
Searching for Axion Stars and Q-Balls with a Terrestrial Magnetometer Network
Developments in Black Hole Research: Classical, Semi-Classical, and Quantum 3
MASTER and Ruffini (151