Is the Supernova Remnant 3C400.2 the Result of a Single Supernova Explosion?

Details Is the Supernova Remnant 3C400.2 the Result of a Single Supernova Explosion? Is the Supernova Remnant 3C400.2 the Result of a Single Supernova Explosion?

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002rmxac..12...93d&link_type=abstract

Ionized Gaseous Nebulae, a Conference to Celebrate the 60th Birthdays of Silvia Torres-Peimbert and Manuel Peimbert, Mexico City

Astronomy and Astrophysics

Astronomy

Instabilities, Line: Profiles, Planetary Nebulae, Stars: Wolf-Rayet, Stars: Mass-Loss

Scientific paper

Using numerical simulations carried out employing a new code YGUAZÚ2D (Raga, Navarro-González, & Villagrán-Muñiz 2000), we find that a single supernova explosion (SN) embedded in a dense medium, occurring close to an interface separating this medium from a less dense medium, is adequate for describing the morphology of the supernova remnant (SNR) 3C400.2.

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