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 …

3C 58 或 3C58 是在 銀河系 中的 脈衝星 （正式名稱為PSR J0205+6449）和 超新星殘骸 （脈衝星風雲），有人認為它可能與1181年的超新星 SN 1181 有關。 然而，有跡象表明它已經有幾千 …

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 …

Here we present observations of 3C58, a young Crab-like nebula believed to be associated with the supernova of 1181 AD. Given this age, 3C58 is presumably powered by one of the …

2014年7月22日 · 3C58 is the remnant of a supernova observed in the year 1181 AD by Chinese and Japanese astronomers. This new Chandra image shows the center of 3C58, which …

Now known as supernova remnant 3C58, the region seen in this false-color image glows in x-rays, powered by a rapidly spinning neutron star or pulsar - the dense remains of the collapsed …

2004年4月19日 · A radio image of the supernova remnant 3C58. The radio nebula is energized by a recently discovered pulsar. The beautiful filamentary structure of the nebula is brought out i …

Chandra's image of 3C58, the remains of a supernova observed on Earth in 1181 AD, shows a rapidly rotating neutron star embedded in a cloud of high-energy particles. The data revealed …

3C 58 或 3C58 是在 银河系 中的 脉冲星 （正式名称为PSR J0205+6449）和 超新星残骸 （脉冲星风云），有人认为它可能与1181年的超新星 SN 1181 有关。 然而，有迹象表明它已经有几千 …

2024年6月20日 · In this image of 3C 58, low-energy X-rays are colored red, medium-energy X-rays are green, and the high-energy band of X-rays is shown in blue. The X-ray data have …