Slide 1 Slide 2 1 Surviving in academia without selling ones soul A panel discussion moderated by K. Nandakumar Univ. of Alberta Slide 3 Sources of pressure l University…

Page 1 Pulsars et Gravitation Ismaël Cognard Chargé de Recherche LPCE / CNRS Orléans [email protected] Page 2 PLAN le décor les pulsars radio la chronométrie…

Slide 1 Neutron Stars Chandrasekhar limit on white dwarf mass Supernova explosions –Formation of elements (R, S process) –Neutron stars –Pulsars Formation of X-Ray…

Slide 1 White Dwarfs and Neutron Stars White dwarfs –Degenerate gases –Mass versus radius relation Neutron stars –Mass versus radius relation –Pulsars, magnetars,…

Can the Merger of a Compact Binary Power a Short-Hard Gamma Ray Burst? Patrick M. Motl (IUK) Ball State University Department of Physics & Astronomy Colloquium, Thursday…

White Dwarf Stars Low mass stars are unable to reach high enough temperatures to ignite elements heavier than carbon in their core become white dwarfs. A white dwarf is the…

White Dwarfs and Neutron Stars White dwarfs Degenerate gases Mass versus radius relation Neutron stars Mass versus radius relation Pulsars, magnetars, X-ray pulsars, X-ray…

Surviving in academia without selling oneâs soul A panel discussion moderated by K. Nandakumar Univ. of Alberta Sources of pressure University âTop Notchâ gets a new president,…

Surviving in academia without selling oneâs soul A panel discussion moderated by K. Nandakumar Univ. of Alberta Sources of pressure University âTop Notchâ gets a new president,…

Chapter Twenty/Twenty-One Questions for the Day What are the end states of stars? How do stars interact? What are the end states of stars? When nuclear fuel is exhausted,…