astro.wikisort.org - Galaxy

Search / Calendar

NGC 681 (also known as the Little Sombrero Galaxy) is an intermediate spiral galaxy in the constellation of Cetus, located approximately 66.5 million light-years from Earth.[1][2][4] The name Little Sombrero Galaxy is a reference to a much larger and earlier observed sombrero-like galaxy designated M104, or the Sombrero Galaxy.

SDSS image of NGC 681
SDSS image of NGC 681

NGC 681
SDSS image showing neighbours
Observation data (J2000 epoch)
ConstellationCetus
Right ascension01h 49m 10.829s[1]
Declination−10° 25′ 35.13″[1]
Redshift0.00587 ± 0.00002[1]
Helio radial velocity1760.4 ± 6.6 km/s[1]
Distance~66.5 million ly (20.39 ± 1.45 Mpc)[1]
Apparent magnitude (V)12[2]
Characteristics
TypeSAB(s)ab
Mass1.9×1010[3] M☉
Mass/Light ratio3.6[3] M☉/L☉
Size~29.07 kpc (diameter)[1]
Apparent size (V)2.70 × 1.8 arcmin[2][4]
Other designations
MCG -02-05-052, PGC 6671[5]

Observation history


NGC 681 was discovered by the German-born British astronomer William Herschel on 28 November 1785 and was later also observed by William's son, John Herschel.[2] John Louis Emil Dreyer, compiler of the first New General Catalogue of Nebulae and Clusters of Stars, described NGC 681 as being a "pretty faint, considerably large, round, small (faint) star 90 arcsec to [the] west" that becomes "gradually a little brighter [in the] middle".[2]


Physical characteristics


The Little Sombrero Galaxy shares many structural similarities with its namesake, M104, although it is smaller, less luminous, and less massive. Its thin, dusty disc is seen almost perfectly edge-on and features a small, very bright nucleus in the center of a very pronounced bulge.[6] Distinctly unlike M104, NGC 681's disc contains many H II regions, where star formation is likely to be occurring.[3][6] The galaxy has a mass of 1.9×1010 M☉, a mass-to-light ratio of 3.6 , and a spiral pattern which is asymmetrical.[3]


    See also



    References


    1. "NGC 681 NASA/IPAC Extragalactic Database Results". ned.ipac.caltech.edu. Retrieved November 2, 2018.
    2. "New General Catalog Objects: NGC 650 - 699". cseligman.com. Retrieved November 2, 2018.
    3. Burbridge, E. M.; G.R., Burbridge; Prendergast, K.H. (1965). "Rotation and Mass of the SA Galaxy, NGC 681". Astrophysical Journal. 142: 154–159. Bibcode:1965ApJ...142..154B. doi:10.1086/148270. hdl:2060/19650010085.
    4. "Revised NGC Data for NGC 681". spider.seds.org. Retrieved November 2, 2018.
    5. "NGC 681". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-19.
    6. Faber, S. M.; Balick, B.; Gallagher, J. S.; Knapp, G. R. (1977). "The neutral hydrogen content, stellar rotation curve, and mass-to-light ratio of NGC 4594, the "Sombrero" galaxy". The Astrophysical Journal. 214: 383–389. Bibcode:1977ApJ...214..383F. doi:10.1086/155260. ISSN 0004-637X.




    На других языках

    [de] NGC 681

    NGC 681 (auch Kleine Sombrerogalaxie) ist eine Balken-Spiralgalaxie vom Hubble-Typ SBab im Sternbild Walfisch südlich der Ekliptik. Sie ist schätzungsweise 79 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 65.000 Lichtjahren. Gemeinsam mit NGC 701, IC 1738 und PGC 6667 bildet sie die NGC 681-Gruppe.
    - [en] NGC 681

    [ru] NGC 681

    NGC 681 (другие обозначения — MCG -2-5-52, IRAS01467-1040, PGC 6671) — галактика в созвездии Кит.


    Текст в блоке "Читать" взят с сайта "Википедия" и доступен по лицензии Creative Commons Attribution-ShareAlike; в отдельных случаях могут действовать дополнительные условия.

    Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.

    2019-2025
    WikiSort.org - проект по пересортировке и дополнению контента Википедии