The Morphologies and Kinematics of Supernova Remnants

被引：27

作者：

Lopez, Laura A. ^{[1
]}

Fesen, Robert A. ^{[2
]}

机构：

[1] Ohio State Univ, 140 W 18th Ave, Columbus, OH 43210 USA

[2] Dartmouth Coll, Wilder Lab 6127, Hanover, NH 03755 USA

来源：

SPACE SCIENCE REVIEWS | 2018年 / 214卷 / 01期

关键词：

Supernova remnants; Supernovae; CASSIOPEIA-A SUPERNOVA; CORE-COLLAPSE SUPERNOVAE; NEUTRON-STAR KICKS; FORMED DENSE SHELL; 3-DIMENSIONAL STRUCTURE; THERMAL CONDUCTION; LIGHT ECHOES; HOT INTERIOR; MODELING W44; RAY-EMISSION;

D O I：

10.1007/s11214-018-0481-x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We review the major advances in understanding the morphologies and kinematics of supernova remnants ( SNRs). Simulations of SN explosions have improved dramatically over the last few years, and SNRs can be used to test models through comparison of predictions with SNRs' observed large-scale compositional and morphological properties as well as the three-dimensional kinematics of ejecta material. In particular, Cassiopeia A-the youngest known core-collapse SNR in the Milky Way-offers an up-close view of the complexity of these explosive events that cannot be resolved in distant, extragalactic sources. We summarize the progress in tying SNRs to their progenitors' explosions through imaging and spectroscopic observations, and we discuss exciting future prospects for SNR studies, such as X-ray microcalorimeters.

引用

页数：26

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