Chandrasekhar limit
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- THE MASS of a STELLAR BLACK HOLE Andrea Massi
- Astronomy 112: the Physics of Stars Class 16 Notes: Post-Main
- Arxiv:2009.01825V2 [Astro-Ph.HE] 8 Apr 2021
- 1 Degenerate Fermi Gas Systems: White Dwarf and Neutron Star (Pulsar)
- Fast Radio Bursts
- The Type Ia Supernova SNLS-03D3bb from a Super-Chandrasekhar-Mass
- Towards a Holographic Description of Pulsar Glitch Mechanism
- The Physics of Chandrasekhar and Super-Chandrasekhar White Dwarfs
- Neutron Stars • Pulsars
- History and Facts About Black Holes
- Fast Radio Bursts: the Last Sign of Supramassive Neutron Stars Heino Falcke1,2,3 and Luciano Rezzolla4,5
- THE COLLAPSING UNIVERSE 5 EXPLODING MATTER 105 the Big Bang 105 the Main Sequence 112 Planetary Nebulas 119 Novas 124 Supernovas 133
- Life Cycle of High Mass Stars Supernovae Neutron Stars, Pulsars, Pulsar Wind Nebulae, Magnetars Quark-Nova Stars Gamma-Ray Bursts (Grbs)
- On the Evolution of Rapidly Rotating Massive White Dwarfs Towards Supernovae Or Collapses
- The Complex Relations Between Supernova Remnants and Neutron Stars Revista Mexicana De Astronomía Y Astrofísica, Vol
- Radio Transients from Accretion-Induced Collapse of White
- Discovery of Pulsars • Discovered by Jocelyn Bell and Tony Hewish in 1967
- Endpoints of Stellar Evolution