NGC 4608 is a barred lenticular galaxy located in the constellation of Virgo. The galaxy was discovered by astronomer William Herschel on March 15, 1784. [3] At about 56 million light-years (17.3 megaparsecs) away, [2] it is a member of the Virgo Cluster. [4]

NGC 4608 is a Lenticular Galaxy in the Virgo constellation. NGC 4608 is situated close to the celestial equator and, as such, it is at least partly visible from both hemispheres in certain times of the year.

NGC 4608 is a barred lenticular galaxy located in the constellation of Virgo. The galaxy was discovered by astronomer William Herschel on March 15, 1784. [3] At about 56 million light-years (17.3 megaparsecs) away, [2] it is a member of the Virgo Cluster .

Inside its B/P bulge, NGC 4608 has a compact, almost circular structure (half-light radius R e ≈ 310 pc, Sérsic n = 2.2) we identify as a classical bulge, amounting to 12.1 per cent of the total light, along with a nuclear star cluster (R e ∼ 4 pc).

We discuss these surprising conclusions, checking for signs of secular evolution, considering bar-forming instabilities, and suggesting, based on N-body simulations, a new mechanism to form bars in spheroids, which includes nonspherical halos.

From Virginia Beach , NGC4608 is visible in the morning sky, becoming accessible around 21:03, when it reaches an altitude of 21° above your eastern horizon. It will then reach its highest point in the sky at 01:44, 63° above your southern horizon. It will be lost to dawn twilight around 05:23, 33° above your western horizon.

Discovered in 1784 by William Herschel with an 18.7-inch f/13 speculum telescope. He called it "pB pL R mbM r." The RNGC (Sulentic and Tifft 1973) notes that this is a 12.5 mag galaxy. Their coded description reads SB,DIFHALOFORMING RG MB TO SHARP BAR&NUC.

NGC 4608 . NGC 4608 is a lenticular galaxy located in the constellation Virgo. Some key stats include:

NGC 4608 is a galaxy in the Virgo Cluster. The Virgo Cluster spans the constellations of Virgo and Coma Berenices and contains approximately 2,000 galaxies, including a number of Messier objects. Galaxy name:

2003年1月6日 · We have performed for the first time in the literature a 2D structural analysis on the barred lenticular and face--on galaxies NGC 4608 and NGC 5701. The results indicate that these galaxies either have never had large disks or their disks were almost completely destroyed by their strong bars, due to secular evolution processes.