NGC 3100 is a Lenticular Galaxy in the Antlia constellation. NGC 3100 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its visual magnitude of 12.47, NGC 3100 is visible with the help of a telescope having an aperture of 8 inches (200mm) or more.

2024年3月2日 · Physical Information: Based on a recessional velocity relative to the Cosmic Microwave Background radiation of 2965 km/sec (and H0 = 70 km/sec/Mpc), NGC 3100 is about 135 to 140 million light-years away. Given that and its apparent size of about 3.7 by 2.1 arcmin (from the images below), the galaxy is about 145 to 150 thousand light-years across.

The Carnegie-Irvine Galaxy Survey (CGS) Data Products . Images • summary from image atlas • original FITS images (B, V, R, I) • color-composite image (original) • color-composite image (star-cleaned) • stacked image • structure maps (B, V, R, I) • color index maps (B-R, R-I) Radial Profiles

2023年5月1日 · We present Australia Compact Telescope Array (ATCA) 21-cm observations of the nearby low-excitation radio galaxy (LERG) NGC 3100. This is the brightest galaxy of a loose group and hosts a young (∼ 2 Myr) radio source.

< NGC List NGC 3100. NGC 3100 is a lenticular galaxy located in the constellation of Antlia. The NGC is a catalog of 7,840 nebulae, star clusters, and galaxies. Here are the key stats on NGC 3100:

NGC 3100 (također poznat kao ESO 435-30, MCG -5-24-18, NGC 3103 i PGC 28960) je prečkasta spiralna galaksija koja je udaljena oko 121 miliona sg od Zemlje i nalazi se u …

NGC 3100 is an Active Galactic Nuclei/Nucleus located in the constellation of Antlia in the southern hemisphere. NGC 3100 is called NGC 3100 in the New General Catalogue (NGC). This catalogue is a list of deep space objects compiled by John Louis Emil Dreyer in 1888 to update John Herschel's earlier work.

2017年12月18日 · A kinematics modelling of molecular gas in the centre of NGC 3100, a FRI radio galaxy hosted by a S0 galaxy at redshift z = 0.0088. The inner region of NGC 3100 has been observed with ALMA at Band 6 during Cycle 3. The CO(2-1) 230-GHz line (rest-frequency) was clearly detected.

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 …

Redshift-Distance Survey of Early-Type Galaxies: Spectroscopic Data We present central velocity dispersions and Mg2 line indicesfor an all-sky sample of ~1178 elliptical and S0 galaxies, of which 984had no previous measures.