NGC 5683 is a type S0-a lenticular galaxy with a bar [1] located in the Boötes constellation. [2] It is 513 million light-years away from the Solar System [3] and has an approximate diameter of 256,000 light-years meaning it is larger compared to the Milky Way. [3] NGC 5683 was discovered by George Johnstone Stoney on April 13, 1850. [4]

NGC 5683 (NGC5683) is a seyfert 1 galaxy that has a distance from Earth of light years. It can be found in the constellation of Boötes.

NGC 5683 is a Lenticular Galaxy in the Boötes constellation. NGC 5683 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its visual magnitude of 16.08, NGC 5683 is visible only through long exposure photography.

2002年5月18日 · NGC 5683 is the host of Supernova 2002 db, and it is a Barred Spiral Galaxy at a considerably greater distance that the other two galaxies. Quasi Stellar Object HB-89 1432+489 is magnitude 19.2 and has a red shift of 1.94, giving a distance estimate of …

Arp, C.H., Khachkyan, É.E. Markaryan 474 (NGC 5683) — A Seyfert galaxy of type one (Sy 1). Astrophysics 9, 308–311 (1973). https://doi.org/10.1007/BF01002515. Anyone you share the following link with will be able to read this content: Provided by the Springer Nature SharedIt content-sharing initiative.

NGC 5683 est une très vaste et lointaine galaxie lenticulaire située dans la constellation du Bouvier. Sa vitesse par rapport au fond diffus cosmologique est de 11 105 ± 11 km/s, ce qui correspond à une distance de Hubble de 164 ± 11 Mpc (∼535 millions d'al) [1]. NGC 5683 a été découverte par le physicien irlandais George Stoney en 1850.

This month, we have some time on the C2PU 1 meter deltagraph. As usual, Serge Brunier started with some GAIA survey for the observatory before imaging. The target was the seyfert galaxy NGC 5683 (the...

NGC 5683 (aliaj indikoj — MCG 8-27-3, MK 474, ZWG 248.9, KUG 1433+488, NPM1G +48.0275, PGC 52114) estas galaksio en konstelacio Bovisto. Ĉi tiu objekto estis jam en la originala …

An Extended FUSE Survey of Diffuse O VI Emission in the Interstellar Medium We present a survey of diffuse O VI emission in the interstellar medium(ISM) obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE).Spanning 5.5 yr of FUSE observations, from launch through 2004 December,our data set consists of 2925 exposures along 183 …

Media in category "NGC 5683" The following 3 files are in this category, out of 3 total.