NGC 959 is a spiral galaxy in the northern constellation of Triangulum. [10] It was discovered on 9 November 1876 by French astronomer Édouard Stephan. [9] This galaxy is located at a distance of 36 million light years and is receding with a heliocentric radial velocity of 596 km/s. [2] It is a member of the NGC 1023 Group of galaxies. [4]

ngc 959 是三角座的一个星系。 维基共享资源上的相关多媒体资源：ngc 959. ned – ngc 959; seds – ngc 959; simbad – ngc 959; vizier – ngc 959

是 三角座 的一個 星系。

2013年7月2日 · NGC 959 is a spiral galaxy in Triangulum. Its distance is an unknown, at least to any degree of accuracy. Redshift puts it at only 17 million light-years. This does rather closely agree to the redshift of NGC 925 that it is considered related to and I imaged back in 2009 http://www.spacebant...53&d=1280601739 . Non redshift distance estimates ...

NGC 959 is a spiral galaxy in Triangulum. Its distance is an unknown, at least to any degree of accuracy. Redshift puts it at only 17 million light-years. This does rather closely agree to the redshift of NGC 925 that it is considered related to and I imaged back in 2009 http://www.spacebanter.com/attachment.php?attachmentid=3053&d=1280601739 .

2009年10月29日 · We present a method to estimate and map the two-dimensional distribution of dust extinction in the late-type spiral galaxy NGC 959 from the theoretical and observed flux ratio of optical V and mid-IR (MIR) 3.6 μm images.

NGC 959，1876年让·玛琏·爱德华·史提芬发现的星系。

NGC 959 . NGC 959 is a late spiral galaxy located in the constellation Triangulum. Some key stats include:

NGC 959 est une petite galaxie spirale rapprochée, peut-être de type magellanique 1, située dans la constellation du Triangle. Sa vitesse par rapport au fond diffus cosmologique est de 378 ± 15 km/s (378 ± 15) km/s, ce qui correspond à une distance de …

NGC 959 is a Spiral Galaxy in the Triangulum constellation. NGC 959 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its visual magnitude of 12.38, NGC 959 is visible with the help of a telescope having an aperture of 8 inches (200mm) or more.

R/B-band color composite image from the Second Digitized Sky Survey (DSS2), measuring 10 arcminutes across. Click and drag the chart above to pan around the sky, or use the mouse wheel to zoom. Click to enlarge. From Virginia Beach , NGC959 will become visible at around 19:04 (EST), 47° above your western horizon, as dusk fades to darkness.

NGC 959 是 三角座 的一個 星系。

NGC 959. Contents. Images; Related articles; Related links; Groups; Images. Upload your image DSS Images Other Images Related articles. The Molecular Interstellar Medium of Dwarf Galaxies on Kiloparsec Scales: A New Survey for CO in Northern, IRAS-detected Dwarf Galaxies

NGC 959 ripresa dal Telescopio spaziale Hubble. NGC 959 ha una classe di luminosità IV-V e presenta una larga riga a 21 cm dell'idrogeno neutro. [2] Nella galassia sono presenti anche regioni di idrogeno ionizzato. [2]Le nitide immagini riprese dal Telescopio spaziale Hubble hanno permesso di comprendere un po' meglio la struttura di questa piccola galassia.

Q1040504 SIMBAD ID: NGC 959. The following 3 files are in this category, out of 3 total.

Download scientific diagram | starlight spectral analysis of NGC 520 (Star-Forming), NGC 959 (Composite), NGC 5838 (AGN/LINER) from top to bottom.

NGC 959 este o galaxie spirală situată în constelația Triunghiul. [6] [7] [8] A fost descoperită în 9 noiembrie 1876 de către Édouard Stephan ⁠(d). [9] Se află la o distanță de 10,96 megaparseci de Pământ. [10]

NGC 949 fa parte del Gruppo di NGC 1023 situato nel Superammasso della Vergine, detto anche Superammasso locale. Questo gruppo comprende le galassie NGC 891 , NGC 925 , NGC 959 , NGC 1003 , NGC 1023 , NGC 1058 e IC 239 .

NGC 959 (također poznat kao IRAS 02293+3516, MCG 6-6-51, PGC 9665 i UGC 2002) je spiralna galaksija koja je udaljena oko 27 miliona sg od Zemlje i nalazi se u sazviježđu Trokut. …