3C 58 or 3C58 is a pulsar (designation PSR J0205+6449) and supernova remnant (pulsar wind nebula) within the Milky Way. The object is listed as No. 58 in the Third Cambridge Catalogue …

How unique are pulsar wind nebulae models? Implementation of a multi-parameter, automatic fitting for time-dependent spectra. Want a reference added? Send a bibtex entry to the TeVCat …

RADIO IMAGES OF 3C 58: EXPANSION AND MOTION OF ITS WISP M. F. Bietenholz Department of Physics and Astronomy, York University, 4700 Keele Street, Toronto, ON M3J …

2006年3月8日 · New 1.4 GHz VLA observations of the pulsar-powered supernova remnant 3C 58 have resulted in the highest quality radio images of this object to date. The images show …

2024年6月24日 · nasa公布的3c 58图片系以x射线和可见光显示。 在超新星残骸的中心是一颗快速旋转的中子星（脉冲星），它呈现出明亮的白色物体，形状有点拉长。 图片中蓝色和紫色的 …

3C58 is the remnant of a supernova observed in the year 1181 by Chinese and Japanese astronomers. A long look by Chandra shows that the central pulsar - a rapidly rotating neutron …

2024年6月20日 · 超新星遗迹 3C 58 的中心包含一颗旋转的中子星，称为 PSR J0205+6449。 天文学家研究了这颗中子星和其他类似的中子星，以探究这些非常致密的物体内部物质的性质。 …

2024年6月20日 · The supernova remnant 3C 58 contains a spinning neutron star, known as PSR J0205+6449, at its center. Astronomers studied this neutron star and others like it to probe the …

2021年9月21日 · 【 NASAのX線観測衛星「チャンドラ」がX線の波長で観測した超新星残骸「3C 58」（疑似カラー）（Credit: NASA/CXC/SAO/P.Slane et al.）】 1181年の超新星について …

This historical supernova explosion most likely left behind the synchrotron nebula 3C 58 (supernova remnant G130.7+3.1), a nebula produced by the wind of a fast-spinning neutron …