Early evolution of spherical ejecta expanding into the circumstellar matter at ultra-relativistic speeds

Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena

Scientific paper

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5 pages, 2 figures, accepted for publication in PASJ

Scientific paper

We present a new self-similar solution describing early evolution of an
ultra-relativistic flow resulting from a collision of homologously expanding
spherical ejecta with the circumstellar matter, in which a shock wave
propagates in the circumstellar matter while a weak discontinuity propagates in
the ejecta at the sound speed

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