NGC 3620 is a Barred Spiral Galaxy in the Chamaeleon constellation. NGC 3620 is situated close to the southern celestial pole and, as such, it is easilty visible for most part of the year from the southern hemisphere. Given its B magnitude of 15.9, NGC 3620 is visible only through long exposure photography.

The cluster has an apparent size of 1.2 by 1 arcmin and is only about 7 light years in diameter, but the surrounding nebula has an apparent size of about 8 by 3.7 arcmin, which corresponds to about 45 light years. LEDA lists NGC 3603 as a cluster with the designation PGC 3518662, but a search of the database for that designation returns no result.

NGC 3620 is a Spiral Galaxy located in the constellation of Chamaeleon in the southern hemisphere. NGC 3620's distance from Earth is 58,626,608.89 light years.

IC 2631 (Ced 112) is a brilliant blue reflection nebula surrounding the young star, HD973000, about 500 light years distant in the southern constellation of Chamaeleon, the Chamaeleon cloud complex is a large region of gas and dust where new stars are forming. The dust partially or nearly totally obscures the stars within and behind it.

2022年7月5日 · The SIMBAD astronomical database provides basic data, cross-identifications, bibliography and measurements for astronomical objects outside the solar system.

NGC 3620 est une galaxie spirale barrée située dans la constellation du Caméléon. Sa vitesse par rapport au fond diffus cosmologique est de 1 812 ± 31 km/s, ce qui correspond à une distance de Hubble de 26,72 ± 1,93 Mpc (∼87,1 millions d' al) 1.

NGC 3632 (also known as Caldwell 40) and NGC 3626[6] is an unbarred lenticular galaxy [5] and Caldwell object in the constellation Leo. It was discovered by William Herschel, on 14 March 1784. It shines at magnitude +10.6 [6] /+10.9. Its celestial …

NGC 3620 ist eine Balken-Spiralgalaxie vom Hubble-Typ SBab im Sternbild Chamäleon am Südsternhimmel, die schätzungsweise 66 Millionen Lichtjahre von der Milchstraße entfernt ist.

2009年8月1日 · Two new detections are reported: a kilomaser with an isotropic luminosity L_ (H_ (2)O) ~ 5 L_☉ in NGC 3620 and a maser with about twice this luminosity in the merger system NGC 3256. The...

Download scientific diagram | Observing parameters for the interferometric continuum maps of NGC 3256 and NGC 3620. from publication: New H_ (2)O masers in Seyfert and FIR bright galaxies: III.