
NGC 7492 - Wikipedia
NGC 7492 is a globular cluster [1] in the constellation Aquarius. It was discovered by the astronomer William Herschel on September 20, 1786. [5] .
NGC 7492 (Gary Imm) - AstroBin
This globular star cluster is located 80,000 light years away in the constellation of Aquarius at a declination of -16 degrees. It is a magnitude 10.5 cluster which spans 4 arc-minutes in our …
NGC 7492 - 华文百科
NGC 7492 是 星座 水瓶座 中的 球状簇。 它是由天文学家 威廉·赫歇尔(William Herschel) 于1786年9月20日发现的。 它居住在 银河系 的郊区,大约80,000光年,是太阳和星系中心之间 …
NGC 7492 - Globular Cluster in Aquarius - TheSkyLive.com
NGC 7492 is a Globular Cluster in the Aquarius constellation. NGC 7492 is situated close to the celestial equator and, as such, it is at least partly visible from both hemispheres in certain …
[1305.4837] Variable stars in the globular cluster NGC 7492. New ...
2013年5月21日 · We have performed a photometric V, R, I CCD time-series analysis with a baseline of ~8 years of the outer-halo globular cluster NGC 7492 with the aim of searching for …
NGC 7492 - Wikiwand
NGC 7492 is a globular cluster in the constellation Aquarius. It was discovered by the astronomer William Herschel on September 20, 1786. It resides in the outskirts of the Milky Way, about …
Mass Segregation and Tidal Tails of the Globular Cluster NGC 7492
2004年9月2日 · We present a wide field CCD photometric study of Galactic globular cluster NGC 7492. The derived VR color-magnitude diagram extends down to about 3.5 mag below the …
NGC 7492 - Students for the Exploration and Development of Space
NGC 7492 is one of the outlying globular clusters of our Milky Way galaxy, at its distance of about 84,000 light-years from us, and 81,200 light-years from the Galactic Center. As its …
NGC 7492 | Star Clusters | Aquarius Constellation | Go Astronomy
NGC 7492 is a globular star cluster located in the constellation Aquarius . NGC 7492 is magnitude 11.29 *, and is 4.2' in size. For reference, the full moon is 30' (arc minutes) or 0.5° in size.
NGC 7492 - University of Queensland
Surface density Proper motions Radial velocities Remnant fraction Mass-to-light ratio