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Interstellar matter, star birth and star death

The gas and dust between the stars, how stars form and how exoplanets were found, the main sequence and what follows it, then white dwarfs, supernovae, neutron stars and pulsars.

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  • Anverso association
    Reverso a loose group of young stars whose spectral types, motions, and positions in the sky indicate a common origin
  • Anverso baryon cycle
    Reverso the cycling of mass in and out of the interstellar medium, including accretion of gas from intergalactic space, loss of gas back into intergalactic space, and conversion of interstellar gas into stars
  • Anverso Chandrasekhar limit
    Reverso the upper limit to the mass of a white dwarf (equals 1.4 times the mass of the Sun)
  • Anverso cosmic rays
    Reverso atomic nuclei (mostly protons) and electrons that are observed to strike Earth’s atmosphere with exceedingly high energies.
  • Anverso degenerate gas
    Reverso a gas that resists further compression because no two electrons can be in the same place at the same time doing the same thing (Pauli exclusion principle)

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Licencia
Creative Commons Attribution 4.0 International CC-BY-4.0
Atribución
Source : https://openstax.org/books/astronomy/pages/preface — Licence : Creative Commons Attribution 4.0 International (https://creativecommons.org/licenses/by/4.0/)
Fuente
OpenStax — Astronomy (first edition)
Obtenido el
Tema
Astronomía
Idioma
English
Versión
3
Actualizado el

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