NGC 2419 (also known as Caldwell 25) is a globular cluster in the constellation Lynx. It was discovered by William Herschel on December 31, 1788. [7] NGC 2419 is at a distance of about 300,000 light years from the Solar System and at the same distance from the Galactic Center.

1999年10月7日 · NGC 2440 is another planetary nebula ejected by a dying star, but it has a much more chaotic structure than NGC 2346. The central star of NGC 2440 is one of the hottest known, with a surface temperature near 200,000 degrees Celsius.

NGC 2449 est une galaxie spirale située dans la constellation des Gémeaux. Sa vitesse par rapport au fond diffus cosmologique est de 5 070 ± 13 km/s, ce qui correspond à une distance de Hubble de 74,8 ± 5,2 Mpc (∼244 millions d'al) [1]. NGC 2449 a été découverte par l'astronome français Édouard Stephan en 1874 [3].

NGC 2449 este o galaxie LINER situată în constelația Gemenii. [3] [4] [5] A fost descoperită în 18 ianuarie 1874 de către Édouard Stephan ⁠(d). [6]

Media in category "NGC 2449" The following 3 files are in this category, out of 3 total.

NGC 2449 is a Barred Spiral Galaxy in the Gemini constellation. NGC 2449 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its B magnitude of 14.3, NGC 2449 is visible with the help of a telescope having an aperture of 14 inches (350mm) or more.

NGC 2442 and NGC 2443 are two parts of a single intermediate spiral galaxy, commonly known as the Meathook Galaxy or the Cobra and Mouse. [3] It is about 50 million light-years away in the constellation Volans.

NGC 4449, also known as Caldwell 21, is an irregular Magellanic type galaxy in the constellation Canes Venatici, being located about 13 million light-years away. [3] It is part of the M94 Group or Canes Venatici I Group that is relatively close to the Local Group hosting our Milky Way galaxy.

2023年8月14日 · Based on a recessional velocity of 4890 km/sec, NGC 2449 is about 225 million light-years away. Given that and its apparent size of 1.3 by 0.6 arcmin, it is about 85 thousand light-years across. Above, a 2.4 arcmin wide closeup of NGC 2449 and part of IC 476

NGC 2441 is a barred spiral galaxy located in the northern constellation of Camelopardalis. [2] Its velocity with respect to the cosmic microwave background is 3492 ± 2 km/s, which corresponds to a Hubble distance of 168.0 ± 11.8 Mly (51.51 ± 3.61 Mpc). [3]