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- Simeis_147 abstract "Simeis 147, also known as the Spaghetti Nebula, SNR G180.0-01.7 or Sharpless 2-240, is a supernova remnant (SNR) that may have occurred in the Milky Way, on the constellation borders of Auriga and Taurus. Discovered in 1952 at the Crimean Astrophysical Observatory using a 25 inch Schmidt-Cassegrain telescope, it is a very difficult object to observe due to its extreme low brightness.The nebulous area is fairly large with an almost spherical shell and filamentary structure. The remnant has an apparent diameter that covers approximately 3°, an estimated distance of approximately 3000 (±350)ly away and an age of approximately 40,000y old.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.".
- Simeis_147 thumbnail Davidedemartin_3.jpg?width=300.
- Simeis_147 wikiPageExternalLink lab_annotations.
- Simeis_147 wikiPageExternalLink catalog&recno=240.
- Simeis_147 wikiPageID "22812755".
- Simeis_147 wikiPageRevisionID "602228073".
- Simeis_147 bV "Unknown".
- Simeis_147 caption "An unknown wavelength image of the supernova remnant nebula from Simeis 147.".
- Simeis_147 constellation Taurus_(constellation).
- Simeis_147 discovery "1952".
- Simeis_147 epoch "J2000".
- Simeis_147 gal "Unknown".
- Simeis_147 hasPhotoCollection Simeis_147.
- Simeis_147 host "Milky way".
- Simeis_147 magV "6.5".
- Simeis_147 name "Simeis 147".
- Simeis_147 progenitor "Unknown".
- Simeis_147 progenitorType "Unknown".
- Simeis_147 snrtype "Mixed-morphology".
- Simeis_147 type "Unknown".
- Simeis_147 subject Category:Auriga_(constellation).
- Simeis_147 subject Category:Sharpless_objects.
- Simeis_147 subject Category:Supernova_remnants.
- Simeis_147 subject Category:Taurus_(constellation).
- Simeis_147 comment "Simeis 147, also known as the Spaghetti Nebula, SNR G180.0-01.7 or Sharpless 2-240, is a supernova remnant (SNR) that may have occurred in the Milky Way, on the constellation borders of Auriga and Taurus. Discovered in 1952 at the Crimean Astrophysical Observatory using a 25 inch Schmidt-Cassegrain telescope, it is a very difficult object to observe due to its extreme low brightness.The nebulous area is fairly large with an almost spherical shell and filamentary structure.".
- Simeis_147 label "Simeis 147".
- Simeis_147 label "Simeis 147".
- Simeis_147 label "Simeis 147".
- Simeis_147 label "Simeis 147".
- Simeis_147 label "Simeis 147".
- Simeis_147 label "Simeis 147".
- Simeis_147 label "シメイズ147".
- Simeis_147 label "西梅兹147".
- Simeis_147 sameAs Simeis_147.
- Simeis_147 sameAs Simeis_147.
- Simeis_147 sameAs Simeis_147.
- Simeis_147 sameAs Simeis_147.
- Simeis_147 sameAs シメイズ147.
- Simeis_147 sameAs Simeis_147.
- Simeis_147 sameAs m.063yd3q.
- Simeis_147 sameAs Q1968201.
- Simeis_147 sameAs Q1968201.
- Simeis_147 wasDerivedFrom Simeis_147?oldid=602228073.
- Simeis_147 depiction Davidedemartin_3.jpg.
- Simeis_147 isPrimaryTopicOf Simeis_147.
