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
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Supernovae, Planetary Nebulae and Supernova Remnants Conference Speakers
Recommended Sessions
- Aeronautical and Aerospace Engineering
- Astrochemistry and Spectroscopy
- Astronomical Computing and Applications
- Astrophysics and Gravitational Waves
- Cosmic Microwave Background and Radiation
- Cosmology and Gravitational Physics
- Dark Matter, Dark Energy, and Black Holes
- Earth and Atmospheric science
- Electromagnetic radiation
- Exoplanets and Planetary Physics
- Galaxies and Big Bang Theory
- Neutrino and Nuclear Astrophysics
- Optical Astronomy and Optoelectronics
- Particle Physics and Higgs Boson
- Physics and Astronomy
- Planets, Comets, Asteroids and Dust
- Space Missions and Satellites
- Stars, Cool Dwarfs, Brown Dwarfs
- Stellar Evolution, Atmospheres and Winds
- Sun, Solar System and Extrasolar Planetary Systems
- Supernovae, Planetary Nebulae and Supernova Remnants
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