Paper:	SN 1987A: 3D Simulations of Collision with the Ring
Volume:	271, Neutron Stars in Supernova Remnants
Page:	379
Authors:	Maeda, K.; Nomoto, K.; Nakasato, N.; Suzuki, T.
Abstract:	We simulate the collision between the ejecta of SN 1987A and circumstellar material, and calculate the X-ray emission. To reproduce observations, the explosion energy and the number density of the HII region are constrained to be ~1.4 x 1051 erg and ~100 amu/cm3, respectively. The density of the hot spot should be similar to that of the ring (~104 amu/cm3) to be consistent with the observed X-ray luminosity. In the near future, the blast wave will reach the dense ring, and the ring will be brightened in X-rays becoming more luminous than 036erg/s.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.046 seconds