NGC 6810 is a spiral galaxy approximately 87 million light-years away from Earth in the constellation of Pavo. [1] NGC 6810 was discovered by John Herschel on July 10, 1834. [3] . It was later added to the New General Catalogue by John Louis Emil Dreyer. This galaxy used to be classified as a Seyfert 2 galaxy, but that is probably incorrect. [4] .

2007年1月22日 · We present the first imaging X-ray observation of the highly inclined (i = 78 deg) Sab Seyfert 2 galaxy NGC 6810 using XMM-Newton, which reveals soft X-ray emission that extends out to a projected...

2007年4月13日 · We present the first imaging X-ray observation of the highly inclined ( i = 78°) Sab Seyfert 2 galaxy NGC 6810 using XMM–Newton, which reveals soft X-ray emission that extends out to a projected height of ∼7 kpc away from the plane of the galaxy.

NGC 6810 is a Spiral Galaxy in the Pavo constellation. NGC 6810 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its visual magnitude of 11.22, NGC 6810 is visible with the help of a telescope having an aperture of 6 inches (150mm) or more.

NGC 6810 (NGC6810) is a seyfert 2 galaxy that has a distance from Earth of 89,575,587.57 light years. It can be found in the constellation of Pavo.

2024年7月6日 · NGC 6810 is a spiral galaxy located 87 million light years away in the constellation of Pavo. The galaxy is classed as an early type, which contrary to one might think the term means it is already in transition towards an elliptical galaxy. Studies have determined that is no activity in the nucleus region.

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

We present the first imaging X-ray observation of the highly inclined (i= 78°) Sab Seyfert 2 galaxy NGC 6810 using XMM–Newton, which reveals soft X-ray emission

2023年8月22日 · Historical Identification: Per Dreyer, NGC 6810 (= GC 4504 = JH 3797, 1860 RA 19 31 43, NPD 148 58.7) is "pretty small, round, very gradually brighter middle". The second IC adds "Not round, but considerably faint, small, considerably extended 170 degrees, stellar nucleus (DeLisle Stewart).

NGC 6810 . NGC 6810 is a early spiral galaxy located in the constellation Pavo. Some key stats include: