NGC 6876 is a Elliptical Galaxy in the Pavo constellation. NGC 6876 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its visual magnitude of 11.54, NGC 6876 is visible with the help of a telescope having an aperture of 8 inches (200mm) or more.

NGC 6876 is a Spiral Galaxy located in the constellation of Pavo in the southern hemisphere. NGC 6876's distance from Earth is 149,575,314.81 light years. NGC 6876 is called NGC 6876 in the New General Catalogue (NGC). This catalogue is a list of deep space objects compiled by John Louis Emil Dreyer in 1888 to update John Herschel's earlier work.

2019年6月14日 · We present the results of a photometric study of the early-type galaxy NGC 6876 and the surrounding globular cluster (GC) system. The host galaxy is a massive elliptical, the brightest of this type in the Pavo Group. According to its intrinsic brightness (Mv ∼ −22.7), it is expected to belong to a galaxy cluster instead of a poor group.

2017年7月25日 · In this work, we present preliminary results for the study of the GC system of NGC 6876, including the color-magnitude diagram, the color distribution, and the spatial, radial and azimuthal distribution for both the entire system and the presumed sub-populations.

2019年7月3日 · We present the results of a photometric study of the early-type galaxy NGC 6876 and the surrounding globular cluster system (GCS). The host galaxy is a massive elliptical, the brightest of this type in the Pavo Group.

We present the results of a photometric study of the early-type galaxy NGC 6876 and the surrounding globular cluster (GC) system. The host galaxy is a massive e

2021年5月9日 · The Spiral NGC 6872 is the main attraction. It is 231 million light years away, 291,000 light years in diameter (3x diameter of Milky Way) and 11.6 magnitude. The Elliptical NGC 6876 is closer at 172 million light years away, 174,000 light years in …

Background-subtracted, mosaicked Spitzer images of the dominant elliptical galaxy NGC 6876 and its companion galaxy NGC 6877 in the 3.6 μm (upper left), 4.5 μm (upper right), 5.8 μm (middle left), and 8.0 μm (middle right) wave bands, respectively.

2019年6月14日 · We present the results of a photometric study of the early-type galaxy NGC 6876 and the surrounding globular cluster (GC) system. The host galaxy is a massive elliptical, the brightest of this type in the Pavo Group. According to its intrinsic brightness (Mv ∼ −22.7), it is expected to belong to a galaxy cluster instead of a poor group.

NGC 6876 - galaxy in the constellation Pavonis Type: E3 - elliptical galaxy The angular dimensions: 2.70'x2.4' magnitude: V=11.3 m; B=12.1 m The surface brightness: 13.2 mag/arcmin 2 Coordinates for epoch J2000: Ra= 20 h 18 m 19.1 s; Dec= -70°51'30" redshift (z): 0.013376 The distance from the Sun to NGC 6876: based on the amount of redshift ...