Supernovae, Planetary Nebulae and Supernova Remnants

A supernova   is a powerful and luminous stellar explosion. A supernova remnant (SNR) is the structure resulting from the explosion of a star in a supernova. The supernova remnant is bounded by an expanding shock wave, and consists of ejected material expanding from the explosion, and the interstellar material it sweeps up and shocks along the way. A planetary nebula, abbreviated as PN is a type of emission nebula consisting of an expanding, glowing shell of ionized gas ejected from red giant stars late in their lives.

 

  • Cosmic rays
  • pulsar wind nebula
  • Hypernova remnants

Related Conference of Supernovae, Planetary Nebulae and Supernova Remnants

April 22-23, 2025

14th International Conference on Separation Techniques & Formulation

Paris, France
April 22-23, 2025

6th International Conference on Physics

Paris, France
June 19-20, 2025

8th International Conference on Astronomy, Astrophysics and Space Science

Budapest, Hungary
June 24-25, 2025

7th International Congress onPhysics

Chicago, USA
October 27-28, 2025

16th International Conference on Exhibition on Lasers, Optics & Photonics

Paris, France
October 27-28, 2025

10th International Conference on Quantum Physics and Mechanics

Aix-en-Provence, France
November 13-14, 2025

18th International Conference on Optics, Photonics & Laser

Paris, France
December 01-02, 2025

9th International Meeting on Fluid Dynamics & Fluid Mechanics

Vancouver, Canada

Supernovae, Planetary Nebulae and Supernova Remnants Conference Speakers

    Recommended Sessions

    Related Journals

    Are you interested in