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Eddington luminosity

  • Mass – Luminosity Relation for Massive Stars

    Mass – Luminosity Relation for Massive Stars

  • Testing Quantum Gravity with LIGO and VIRGO

    Testing Quantum Gravity with LIGO and VIRGO

  • Astronomy 112: the Physics of Stars Class 10 Notes: Applications and Extensions of Polytropes in the Last Class We Saw That Poly

    Astronomy 112: the Physics of Stars Class 10 Notes: Applications and Extensions of Polytropes in the Last Class We Saw That Poly

  • Ultraluminous X-Ray Pulsars

    Ultraluminous X-Ray Pulsars

  • Exceeding the Eddington Limit

    Exceeding the Eddington Limit

  • A Supercomputer Models a Blinking, Impossibly Bright 'Monster Pulsar' 8 September 2016

    A Supercomputer Models a Blinking, Impossibly Bright 'Monster Pulsar' 8 September 2016

  • Models of Hydrostatic Magnetar Atmospheres at High Luminosities

    Models of Hydrostatic Magnetar Atmospheres at High Luminosities

  • Luminous Blue Variables & Mass Loss Near the Eddington Limit

    Luminous Blue Variables & Mass Loss Near the Eddington Limit

  • Supermassive Mass Black Holes

    Supermassive Mass Black Holes

  • Modified Theories and Non-Singular Black Holes

    Modified Theories and Non-Singular Black Holes

  • © in This Web Service Cambridge University

    © in This Web Service Cambridge University

  • Arxiv:1807.06243V1 [Astro-Ph.HE] 17 Jul 2018

    Arxiv:1807.06243V1 [Astro-Ph.HE] 17 Jul 2018

  • Luminosity, Selfgravitation and Nonuniqueness of Stationary Accretion

    Luminosity, Selfgravitation and Nonuniqueness of Stationary Accretion

  • Levitating Atmospheres of Eddington-Luminosity Neutron Stars

    Levitating Atmospheres of Eddington-Luminosity Neutron Stars

  • Massive Pulsars and Ultraluminous X-Ray Sources

    Massive Pulsars and Ultraluminous X-Ray Sources

  • Arxiv:1904.05363V3 [Gr-Qc] 13 Jun 2019

    Arxiv:1904.05363V3 [Gr-Qc] 13 Jun 2019

  • Convection 21 September 2011

    Convection 21 September 2011

  • BIFURCATION in the SHAKURA MODEL∗ Krzysztof Roszkowski

    BIFURCATION in the SHAKURA MODEL∗ Krzysztof Roszkowski

Top View
  • Inaugural Dissertation
  • Eddington Capture Sphere Around Luminous Stars
  • Download This Article in PDF Format
  • Ultraluminous X-Ray Pulsar: Accreting Magnetar?
  • 5 Accretion Flows
  • Accreting, Highly Magnetized Neutron Stars at the Eddington Limit: a Study of the 2016 Outburst of SMC X-3 Filippos Koliopanos1,2 and Georgios Vasilopoulos3
  • Arxiv: Testing the Nature of Dark Compact Objects: a Status Report
  • Cosmology and Extragalactic Astronomy Black Holes Part II
  • Can Accretion Disk Properties Distinguish Gravastars from Black
  • Lecture 7 Evolution of Massive Stars on the Main Sequence and During
  • Black Holes Physics
  • Distinguishing Brans–Dicke–Kerr Type Naked Singularities and Black Holes with Their Thin Disk Electromagnetic Radiation Properties
  • Super-Eddington Accretion Onto Black Holes and Neutron Stars
  • Testing the Nature of Dark Compact Objects: a Status Report
  • Instability & Mass Loss Near the Eddington Limit
  • Stellar Disruption Events Support the Existence of the Black Hole Event Horizon
  • Astronomy 112: the Physics of Stars Class 14 Notes: the Main
  • Introduction Exercise 1


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