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 of Radio Sources. It is located 2° northeast of ε Cassiopeiae and …

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 Team.

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 1P3, Canada Received 2006 January 9; accepted 2006 March 7 ABSTRACT New 1.4 GHz VLA observations of the pulsar-powered supernova remnant 3C 58 have resulted in the highest

Mar 8, 2006 · 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 filamentary structure over the body of the nebula.

Jun 24, 2024 · 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环状物质和漩涡从中子星向多个方向向外延伸，很像章鱼与其手臂的形状。

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 star formed in the supernova event - is surrounded by a bright torus of X-ray emission.

Jun 20, 2024 · 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。 一项利用美国宇航局的钱德拉 X 射线天文台和欧空局的 XMM-Newton 进行的新研究表明，中子星的内部可能包含一种在宇宙中其他地方找不到的超致密物质。 在这张 3C 58 的图像中，低能 X 射线显示为红色，中能 X 射线显示为绿色，高能 X 射线带显示为蓝色。 X 射线数据与数字化巡天的光学 …

Jun 20, 2024 · 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 nature of matter inside these very dense objects.

Sep 21, 2021 · 【 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は、これまでカシオペヤ座の方向にある超新星残骸 「3C 58」 が対応する天体ではないかと考えられ …

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 star, the pulsar J 0205+6449. 3C 58 is very similar to the Crab Nebula in age, distance, size, and morphology, but much less luminous.