Most interesting was the discovery of an extensive UV disk around the diminutive Sm galaxy NGC 4625, which suggests that the galaxy is currently forming most of its stars (Gil de Paz et al.
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We then traced how the morphometry is degraded in each z … It has the designation NGC 4374 in the New General Catalogue.Messier Objects: Guide to the Bright Galaxies, Nebulae and Clusters Listed in the Messier CatalogueThis website uses cookies to personalise content and ads, and to analyse user traffic. With over a thousand known members, the cluster spans an area of the sky about 5 by 3 degrees in size. The Virgo Cluster is the closest large cluster of galaxies to the Milky Way. Apart from that the galaxy shows evidence for a kinematically decoupled core. NGC 4458 in the Virgo cluster of galaxies. Credit: Messier 84 (M84) is an elliptical or lenticular galaxy located in the inner region of the Virgo Cluster, in the constellation Virgo. Begin typing the name of a town near to you, and then select the town from the list of options in Virgo (RA 12 21 54.9, Dec +04 28 24) Click on the image (below) or the NGC link (above) for more information
In contrast, the cold central disc of NGC 4478 is younger, richer in metals and less overabundant than the main body of the galaxy.
IC 4458 - Spiral Galaxy is classified as Spiral (SAbc) according to the Hubble and de Vaucouleurs galaxy morphological classification. The string of galaxies – which also includes NGC 4477, NGC 4473, NGC 4461, NGC 4458, NGC 4438 and NGC 4435 – occupies more than a full … Messier 86 (M86) is an elliptical or lenticular galaxy located in the Virgo Cluster, in the southern constellation Virgo. Line strength maps of 48 elliptical and lenticular galaxies We present absorption line strength maps of 48 representative ellipticaland lenticular galaxies obtained as part of a survey of nearby galaxiesusing our custom-built integral-field spectrograph, SAURON, operating onthe William Herschel Telescope. … This galaxy has been found to be uniformly old despite being counter-rotating.
In contrast, the cold central disc of NGC 4478 is younger, richer in metals and less overabundant than the main body of the galaxy. which appear below. The galaxy lies at an approximate distance of 60 million light years from Earth and has an apparent magnitude of 10.1. The galaxy NGC 4458. Position: 13° 14' 29.9"
ESA uses cookies to track visits to our website only, no personal information is collected. Red-band image from the Second Digitized Sky Survey (DSS2), measuring 10 arcminutes across. The Sombrero Galaxy (also known as Messier Object 104, M104 or NGC 4594) is a lenticular galaxy ‹The template Failed verification is being considered for merging.› [ failed verification ] in the constellation borders of Virgo and Corvus, being about 9.55 megaparsecs (31.1 million light-years) from Earth. Click and drag the chart above to pan around the sky, or use the mouse wheel to zoom. NGC 4762 is an edge-on SB0bc galaxy with a very small classical-bulge-to-total ratio of B/T = 0.13 ± 0.02. Hubble's "eye" is so sharp that it was able to pick out the fuzzy globular clusters, which, at that distance, look like individual stars bunched up around the galaxies, instead of groupings of stars.
This galaxy has been found to be uniformly old despite being counter-rotating. NGC 4452 is an edge-on SB0 galaxy with an even tinier pseudobulge-to-total ratio of PB/T = 0.017 ± 0.004. Hubble's "eye" is so sharp that it was able to pick out the fuzzy globular clusters, which, at that distance, look like individual stars bunched up around the galaxies, instead of groupings of stars.
For more information including contact details, NGC 4435 is a barred lenticular galaxy currently interacting with NGC 4438. Virgo cluster galaxy NGC 4458. Red-band image from the Second Digitized Sky Survey (DSS2), measuring 10 arcminutes across. NGC 4458 is a member of Markarian's Chain which is part of the Virgo Cluster.
Begin typing the name of a town near to you, and then select the town from the list of options NGC 4458 and NGC 4461 are both Interacting with each other. However, NGC 7029 is not boxy throughout: it shows evidence of a small inner disk and hence is disky at small radii. The two are likely interacting gravitationally, accounting for the peculiar appearance of NGC 3718.
The counter-rotating central disc of NGC 4458 is found to have similar properties to the decoupled cores of bright ellipticals.