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Simeis 147 : ウィキペディア英語版
Simeis 147

Simeis 147, also known as the Spaghetti Nebula, SNR G180.0-01.7 or Sharpless 2-240, is a supernova remnant (SNR) in the Milky Way, straddling the border between the constellations Auriga and Taurus. Discovered in 1952 at the Crimean Astrophysical Observatory using a 25-inch Schmidt-Cassegrain telescope, it is difficult to observe due to its extremely low brightness.
The nebulous area is fairly large with an almost spherical shell and filamentary structure.〔(【引用サイトリンク】url=http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-ref=VIZ52b391ab3a6e&-out.add=.&-source=VII/20/catalog&recno=240 )〕 The remnant has an apparent diameter of approximately 3 degrees, an estimated distance of approximately 3000 (±350) light-years, and an age of approximately 40,000 years.〔(【引用サイトリンク】url=http://apod.nasa.gov/apod/ap121009.html )
It is believed that after its stellar explosion a rapidly spinning neutron star known as pulsar PSR J0538+2817 was left behind in the nebula core, emitting a strong radio signal.〔(【引用サイトリンク】url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=SIM%20147#lab_annotations )
== References ==


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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