NGC 4344 is a Lenticular Galaxy in the Coma Berenices constellation. NGC 4344 is situated close to the celestial equator and, as such, it is at least partly visible from both hemispheres in …

NGC 4344 is a Spiral Galaxy located in the constellation of Coma Berenices in the northern hemisphere. NGC 4344's distance from Earth is 37,507,983.43 light years.

NGC 4344 este o galaxie lenticulară situată în constelația Părul Berenicei. [6][7][8] A fost descoperită în 14 martie 1784 de către William Herschel. [9] Se află la o distanță de 17 megaparseci de Pământ. [10]

The following 2 files are in this category, out of 2 total. This page was last edited on 6 March 2019, at 11:58. Files are available under licenses specified on their description page.

2022年2月18日 · NED - NASA/IPAC Extragalactic Database : NGC4344 VizieR NGC 4344 IRAS F12210+1749 IRAS 12210+1748 KUG 1221+178 2MASX J12233719+1732150 SDSS J122337.45+173227.2 UGC 7468 Gaia DR2 3946897305178804864 Gaia EDR3 3946897305178804864 Vizier (radius: 5 arcsec)

2021年10月2日 · The SIMBAD astronomical database provides basic data, cross-identifications, bibliography and measurements for astronomical objects outside the solar system.

LEDA/PGC 4344 (NGC 434A) ist eine Linsenförmige Galaxie vom Hubble-Typ SB0/a im Sternbild Tukan am Südsternhimmel. Sie ist schätzungsweise 211 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 75.000 Lichtjahren.

From Redmond , NGC4344 is visible all night. It will become visible at around 20:34 (PDT), 22° above your eastern horizon, as dusk fades to darkness. It will then reach its highest point in the sky at 01:39, 59° above your southern horizon. It will be lost to dawn twilight at around 05:55, 30° above your western horizon.

NGC 4344 est une petite galaxie lenticulaire située dans la constellation de la Chevelure de Bérénice. Sa vitesse par rapport au fond diffus cosmologique est de 1 473 ± 23 km/s, ce qui correspond à une distance de Hubble de 21,7 ± 1,6 Mpc (∼70,8 millions d' al) 1.

Related articles Palomar/Las Campanas Imaging Atlas of Blue Compact Dwarf Galaxies. II. Surface Photometry and the Properties of the Underlying Stellar PopulationWe present the results from an analysis of surface photometry of B, R,and Hα images of a total of 114 nearby galaxies (vhelio<4000 km s-1) drawn from the Palomar/LasCampanas Imaging Atlas of blue compact dwarf (BCD) galaxies ...