NGC 5265 is a Galaxy in the Canes Venatici constellation. NGC 5265 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its B magnitude of 14.9, NGC 5265 is visible with the help of a telescope having an aperture of 20 inches (500mm) or more.

2023年11月3日 · NGC 5265 -- Radio Galaxy The astronomical object called NGC 5265 is a Radio Galaxy: Origin of the objects types : (Ref) Object type as listed in the reference "Ref" (acronym) Object type linked to the acronym according to the original reference Anterior to 2007, before we can link the objet type to a reference, or given by the CDS team in some ...

< NGC List NGC 5265. NGC 5265 is a barred spiral galaxy located in the constellation of Canes Venatici. The NGC is a catalog of 7,840 nebulae, star clusters, and galaxies. Here are the key stats on NGC 5265:

Object NGC 5265 is located exactly in the center of the picture. NGC 5265 - galaxy in the constellation Canum Venaticorum Type: SBcd - spiral galaxy with bar The angular dimensions: 0.70'x0.6' magnitude: V=13.9 m; B=14.6 m The surface brightness: 12.8 mag/arcmin 2 Coordinates for epoch J2000: Ra= 13 h 40 m 9 s; Dec= 36°51'41" redshift (z): 0. ...

NGC 5265 (NGC5265) is a radio galaxy that has a distance from Earth of light years. It can be found in the constellation of Canes Venatici.

Guides to the night sky. Location: Virginia Beach (36.85°N; 75.98°W) NGC5265 (Galaxy)

NGC 5265 este o infrared source ⁠(d) situată în constelația Câinii de Vânătoare. [3] [4] [5] A fost descoperită în 1 mai 1785 de către William Herschel. [6]

Revised NGC Data for NGC 5265 Data from Wolfgang Steinicke's Revised NGC and IC Catalog. Object: NGC 5265 (*) Galaxy, type SBcd, in Canes Venatici Right Ascension (2000.0): …

An image database. II. Catalogue between δ=-30deg and δ=70deg. A preliminary list of 68.040 galaxies was built from extraction of35.841 digitized images of the Palomar Sky Survey (Paper I).

NGC 5265 — Yeni Ümumi Kataloqda qeydə alınmış qalaktika. Göy üzündə Tazılar bürcü istiqamətində yerləşir. SBcd tipli qalaktikadır. İngilis astronomu Vilyam Herşel tərəfindən 1785-ci ildə 47.5 sm (18.7 düymə) ölçülü reflektor vasitəsilə kəşf edilmişdir. [5]