PROGENITORS OF RECOMBINING SUPERNOVA REMNANTS

@article{Moriya2012PROGENITORSOR,
  title={PROGENITORS OF RECOMBINING SUPERNOVA REMNANTS},
  author={T. Moriya},
  journal={The Astrophysical Journal},
  year={2012},
  volume={750}
}
  • T. Moriya
  • Published 2012
  • Physics
  • The Astrophysical Journal
  • Usual supernova remnants have either ionizing plasma or plasma in collisional ionization equilibrium, i.e., the ionization temperature is lower than or equal to the electron temperature. However, the existence of recombining supernova remnants, i.e., supernova remnants with ionization temperature higher than the electron temperature, has been recently confirmed. One suggested way to have recombining plasma in a supernova remnant is to have a dense circumstellar medium at the time of the… CONTINUE READING
    17 Citations

    Figures from this paper.

    Supernova Remnants as Clues to Their Progenitors
    • 6
    • PDF
    Numerical Simulations of Supernova Remnant Evolution in a Cloudy Interstellar Medium
    • 16
    • PDF
    The Progenitor of SN 2011ja: Clues from Circumstellar Interaction
    • 15
    • PDF
    Supernova Remnants Interacting with Molecular Clouds: X-Ray and Gamma-Ray Signatures
    • 35
    • Highly Influenced
    • PDF
    Thermal X-ray Spectra of Supernova Remnants
    • 1
    • PDF
    UNRAVELING THE ORIGIN OF OVERIONIZED PLASMA IN THE GALACTIC SUPERNOVA REMNANT W49B
    • 21
    • PDF

    References

    SHOWING 1-10 OF 50 REFERENCES
    New insights into SNR evolution revealed by the discovery of recombining plasmas
    • 10
    • Highly Influential
    • PDF
    Hydrogen-poor superluminous stellar explosions
    • 338
    • PDF
    The evolution of supernovae in circumstellar wind bubbles. II. Case of a wolf-rayet star
    • 72
    • PDF
    DISCOVERY OF STRONG RADIATIVE RECOMBINATION CONTINUA FROM THE SUPERNOVA REMNANT IC 443 WITH SUZAKU
    • 81
    • PDF