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- Q1108639 subject Q1031119.
- Q1108639 subject Q10661.
- Q1108639 subject Q7033664.
- Q1108639 subject Q7152550.
- Q1108639 abstract "NGC 4041 is the New General Catalogue identifier for a spiral galaxy in the northern circumpolar constellation of Ursa Major. It is located an estimated 70 million light years from the Sun. The morphological classification of SA(rs)bc indicates this is a spiral galaxy the lacks a bar; the 'rs' means it has a weakly-formed ring structure, and the 'bc' indicates the spiral arms are moderately to loosely wound.The galaxy is inclined by around 20° to the line of sight from the Earth. It is forming new stars at the estimated rate of 4.10 M⊙ yr−1, which is fairly typical for a galaxy of this morphology. The star formation rate is much higher in the central region, which may be the result of recent merger with a dwarf galaxy within the last 100 million years.This galaxy has no detected activity in the nuclear region. There is a rotating nuclear disk of high brightness at the core that is consistent with the presence of a compact mass of 7007100000000000000♠1+0.6−0.7×107 M⊙. Most likely this is a supermassive black hole (SMBH).On July 29, 1994, the type IIp supernova designated SN 1994W was discovered in this galaxy by Giancarlo Cortini and Mirko Villi. The event reached peak visual magnitude on August 13, and declined thereafter. It was located about 19 arc seconds to the northwest of the nucleus. This supernova was unusual for the exceptionally low quantity of nickel-56 released—indeed, it was the lowest inferred amount measured for any type II supernova as of that date. Based upon a possible detection of X-ray emission from the remnant, this may be a high-luminosity type IIn supernova.NGC 4041 is a member of the LGG 266 galaxy group, along with NGC 4036, IC 758, UGC 7009, and UGC 7019. It is located just 17 arc minutes from NGC 4036, and the two form a pair with a projected separation of around 470 kly (143 kpc).".
- Q1108639 thumbnail NGC_4041_hst_09042_R814G606B450.png?width=300.
- Q1108639 wikiPageWikiLink Q1031119.
- Q1108639 wikiPageWikiLink Q1049029.
- Q1108639 wikiPageWikiLink Q10661.
- Q1108639 wikiPageWikiLink Q1067416.
- Q1108639 wikiPageWikiLink Q1108621.
- Q1108639 wikiPageWikiLink Q115462.
- Q1108639 wikiPageWikiLink Q14534.
- Q1108639 wikiPageWikiLink Q1491746.
- Q1108639 wikiPageWikiLink Q1648748.
- Q1108639 wikiPageWikiLink Q180892.
- Q1108639 wikiPageWikiLink Q22066400.
- Q1108639 wikiPageWikiLink Q2488.
- Q1108639 wikiPageWikiLink Q2490.
- Q1108639 wikiPageWikiLink Q2513.
- Q1108639 wikiPageWikiLink Q40392.
- Q1108639 wikiPageWikiLink Q531.
- Q1108639 wikiPageWikiLink Q5571730.
- Q1108639 wikiPageWikiLink Q605931.
- Q1108639 wikiPageWikiLink Q615925.
- Q1108639 wikiPageWikiLink Q6709611.
- Q1108639 wikiPageWikiLink Q7033664.
- Q1108639 wikiPageWikiLink Q7152550.
- Q1108639 wikiPageWikiLink Q724913.
- Q1108639 wikiPageWikiLink Q8918.
- Q1108639 name "NGC 4041".
- Q1108639 names "2".
- Q1108639 type Place.
- Q1108639 type CelestialBody.
- Q1108639 type Galaxy.
- Q1108639 type Location.
- Q1108639 type Place.
- Q1108639 type Thing.
- Q1108639 type Q318.
- Q1108639 comment "NGC 4041 is the New General Catalogue identifier for a spiral galaxy in the northern circumpolar constellation of Ursa Major. It is located an estimated 70 million light years from the Sun. The morphological classification of SA(rs)bc indicates this is a spiral galaxy the lacks a bar; the 'rs' means it has a weakly-formed ring structure, and the 'bc' indicates the spiral arms are moderately to loosely wound.The galaxy is inclined by around 20° to the line of sight from the Earth.".
- Q1108639 label "NGC 4041".
- Q1108639 depiction NGC_4041_hst_09042_R814G606B450.png.
- Q1108639 name "2MASXJ12021217+6208142,IRAS11596+6224 ,LEDA37999,UGC7014,UZCJ120212.2+620814,Z292-61.".
- Q1108639 name "NGC 4041".