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- Q1038026 subject Q1031119.
- Q1038026 subject Q10597.
- Q1038026 subject Q7033665.
- Q1038026 subject Q7152546.
- Q1038026 subject Q9495714.
- Q1038026 abstract "NGC 660 is a peculiar and unique polar-ring galaxy located approximately 45 million light years from Earth in the Pisces constellation. It is the only such galaxy having, as its host, a "late-type lenticular galaxy". It was probably formed when two galaxies collided a billion years ago. However, it may have first started as a disk galaxy that captured matter from a passing galaxy. This material could have, over time, become "strung out" to form a rotating ring.The ring is not actually polar, but rather has an inclination from the plane of the host disk of approximately 45 degrees. The extreme number of pinkish star-forming areas that occurs along the galaxy's ring could be the result of the gravitation interaction caused by this collision. The ring is 50,000 light-years across - much broader than the disk itself - and has a greater amount of gas and star formation than the host ring. This likely indicates a very violent formation. The polar ring contains objects numbering in the hundreds. Many of these are red and blue supergiant stars. The most recently created stars in the ring were just formed approximately 7 million years ago. This indicates that the formation of these stars has been a long process and is still occurring.Data about the dark matter halo of NGC 660 can be extracted by observing the gravitational effects of the dark matter on the disk and ring's rotation. From the core of the disk, radio waves are being emitted. The source of these waves is an area only 21 light years across. This may indicate the presence of a super-cluster of stars located within an area of cloud of gas.The region in the centre has a vast amount of star formation, so luminous that it is considered to be a starburst galaxy.Late in 2012, this polar-ring galaxy produced an enormous outburst having a magnitude of approximately ten times brighter than a supernova explosion. The cause is not certain, but this event may have resulted from a tremendous jet being emenating from galaxy's central black hole.".
- Q1038026 thumbnail NGC_660_Polar_Galaxy_Gemini_Observatory.jpg?width=300.
- Q1038026 type Q1752077.
- Q1038026 wikiPageWikiLink Q1031119.
- Q1038026 wikiPageWikiLink Q10597.
- Q1038026 wikiPageWikiLink Q14534.
- Q1038026 wikiPageWikiLink Q1479861.
- Q1038026 wikiPageWikiLink Q1752077.
- Q1038026 wikiPageWikiLink Q2014003.
- Q1038026 wikiPageWikiLink Q22066400.
- Q1038026 wikiPageWikiLink Q2703.
- Q1038026 wikiPageWikiLink Q615925.
- Q1038026 wikiPageWikiLink Q6634097.
- Q1038026 wikiPageWikiLink Q7033665.
- Q1038026 wikiPageWikiLink Q7152546.
- Q1038026 wikiPageWikiLink Q726611.
- Q1038026 wikiPageWikiLink Q744667.
- Q1038026 wikiPageWikiLink Q8679.
- Q1038026 wikiPageWikiLink Q9495714.
- Q1038026 name "NGC 660".
- Q1038026 names "NGC 660, PGC 6318, LEDA 6318, UGC 1201".
- Q1038026 type "SBa pec / Polar-ring galaxy".
- Q1038026 type Place.
- Q1038026 type CelestialBody.
- Q1038026 type Galaxy.
- Q1038026 type Location.
- Q1038026 type Place.
- Q1038026 type Thing.
- Q1038026 type Q318.
- Q1038026 comment "NGC 660 is a peculiar and unique polar-ring galaxy located approximately 45 million light years from Earth in the Pisces constellation. It is the only such galaxy having, as its host, a "late-type lenticular galaxy". It was probably formed when two galaxies collided a billion years ago. However, it may have first started as a disk galaxy that captured matter from a passing galaxy.".
- Q1038026 label "NGC 660".
- Q1038026 depiction NGC_660_Polar_Galaxy_Gemini_Observatory.jpg.
- Q1038026 name "NGC 660".
- Q1038026 name "NGC660,PGC6318, LEDA 6318,UGC1201".