NGC 3198, also known as Herschel 146 [5] is a barred spiral galaxy in the constellation Ursa Major. It was discovered by William Herschel on 15 January 1788. [6] [3] NGC 3198 is located in the Leo Spur, [3] which is part of the Virgo Supercluster, [7] …

Jan 15, 2019 · In this paper, the density and mass variation with the distance from the center of the galaxy NGC 3198 is studied depending on its observed rotation curve (Rubin et al. 1977). The galaxy NGC 3198 is classified as a spiral type SBc (late type), but in photographs such as Palomar sky, survey prints, the bar is not very prominent.

The galaxy NGC 3198 was discovered on 15 January 1788 by the German-British astronomer William Herschel with his self-built 18.7 inch f/12.8 reflecting telescope in Slough, England. [ 277 ] Distances of this spiral galaxy of the morphological type S_AB range from 11 Mpc to 17 Mpc.

We model the spiral galaxy NGC 3198 as consisting of three “luminous” components, namely the bulge and the stellar and the gaseous disks, which are embedded in a dark halo. To study the properties of luminous and DM in this galaxy, we model the RC in terms of the contributions from the stellar disk, the bulge, the gaseous disk, and the DM ...

NGC 3198 is a Spiral Galaxy in the Ursa Major constellation. NGC 3198 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its visual magnitude of 10.33, NGC 3198 is visible with the help of a binocular with a 80mm aperture or a small telescope.

This object is a weakly barred 10th magnitude spiral galaxy located 50 million light years away in the constellation of Ursa Major. The galaxy is large at a diameter of 140,000 light years. It is 10...

ngc 3198是位于大熊座的一个星系。它的赤经为 1019.9，赤纬为 45° 33′，大小 8.3′。

Mar 13, 2015 · We use recent very extended HI kinematics (out to 48 kpc) along with previous H α kinematics of the spiral galaxy NGC 3198 in order to derive its distribution of dark matter (DM).

The density and mass of the spiral galaxy NGC 3198 have been studied as functions of the distance from the center of galaxy depending on its observed rotation curve. Calculation of density and mass at different radii of the galaxy

NGC 3198, also known as Herschel 146 is a barred spiral galaxy in the constellation Ursa Major. It was discovered by William Herschel on 15 January 1788. NGC 3198 is located in the Leo Spur, which is part of the Virgo Supercluster, and is approximately 47 million light years away. Quick Facts Observation data (J2000 epoch), Constellation ...