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- 1E161348-5055 abstract "1E161348-5055 or 1E 161348-5055 is a neutron star found in the centre of RCW103 supernova remnant. It is a periodic X-Ray source with a period of 6.67 hours. It is approximately 2000 years old. It is 10,000 light years away in the constellation Norma.The star was discovered by the Einstein Observatory.This star is unusual because of its rotation period of 6.7 hours. Its period is too long for a star of 2000 years, which should be rotating thousands of times faster. Instead, it is behaving more like a multi-million-year-old star. Another oddity occurred between October 1999 and January 2000. The star became 50 times brighter. The flare has faded since its peak but has not returned to its pre-1999 level. Two theories have been put forward to explain these phenomena.The first is that the star possesses a massive magnetic field. This strong field would brake against the debris disk left behind by the supernova, which has thus far been unknown to science. This theory would account for the slower than expected rotation but not for the increase in brightness.An alternate explanation is that the star has a low-mass X-ray binary. The companion star would orbit in an elongated orbit. When the companion is close to the neutron star, it would feed mass into it, creating the increased brightness. The drag created by the companion on the neutron star's magnetic field would also slow the rotation of the neutron star. If this scenario is the case, it is the youngest such system yet observed.".
- 1E161348-5055 wikiPageExternalLink Supernova_Leaves_Behind_Mysterious_Object_999.html.
- 1E161348-5055 wikiPageID "6048636".
- 1E161348-5055 wikiPageLength "2591".
- 1E161348-5055 wikiPageOutDegree "13".
- 1E161348-5055 wikiPageRevisionID "661025359".
- 1E161348-5055 wikiPageWikiLink Category:Neutron_stars.
- 1E161348-5055 wikiPageWikiLink Category:Norma_(constellation).
- 1E161348-5055 wikiPageWikiLink Constellation.
- 1E161348-5055 wikiPageWikiLink Debris_disk.
- 1E161348-5055 wikiPageWikiLink Einstein_Observatory.
- 1E161348-5055 wikiPageWikiLink Low-mass_X-ray_binary.
- 1E161348-5055 wikiPageWikiLink Magnetic_field.
- 1E161348-5055 wikiPageWikiLink Neutron_star.
- 1E161348-5055 wikiPageWikiLink Norma_(constellation).
- 1E161348-5055 wikiPageWikiLink RCW103.
- 1E161348-5055 wikiPageWikiLink Rotation_period.
- 1E161348-5055 wikiPageWikiLink Supernova_remnant.
- 1E161348-5055 wikiPageWikiLink X-Ray.
- 1E161348-5055 wikiPageWikiLink X-ray.
- 1E161348-5055 wikiPageWikiLink X-ray_binary.
- 1E161348-5055 wikiPageWikiLinkText "1E 161348-5055".
- 1E161348-5055 wikiPageWikiLinkText "1E161348-5055".
- 1E161348-5055 hasPhotoCollection 1E161348-5055.
- 1E161348-5055 wikiPageUsesTemplate Template:Cite_conference.
- 1E161348-5055 wikiPageUsesTemplate Template:Cite_journal.
- 1E161348-5055 wikiPageUsesTemplate Template:Refbegin.
- 1E161348-5055 wikiPageUsesTemplate Template:Refend.
- 1E161348-5055 wikiPageUsesTemplate Template:Reflist.
- 1E161348-5055 wikiPageUsesTemplate Template:Stars_of_Norma.
- 1E161348-5055 subject Category:Neutron_stars.
- 1E161348-5055 subject Category:Norma_(constellation).
- 1E161348-5055 hypernym Star.
- 1E161348-5055 type Article.
- 1E161348-5055 type Star.
- 1E161348-5055 type Article.
- 1E161348-5055 comment "1E161348-5055 or 1E 161348-5055 is a neutron star found in the centre of RCW103 supernova remnant. It is a periodic X-Ray source with a period of 6.67 hours. It is approximately 2000 years old. It is 10,000 light years away in the constellation Norma.The star was discovered by the Einstein Observatory.This star is unusual because of its rotation period of 6.7 hours. Its period is too long for a star of 2000 years, which should be rotating thousands of times faster.".
- 1E161348-5055 label "1E161348-5055".
- 1E161348-5055 sameAs m.0fmgx4.
- 1E161348-5055 sameAs 1E_161348-5055.
- 1E161348-5055 sameAs Q4029723.
- 1E161348-5055 sameAs Q4029723.
- 1E161348-5055 wasDerivedFrom 1E161348-5055?oldid=661025359.
- 1E161348-5055 isPrimaryTopicOf 1E161348-5055.