NGC 7592 is an interacting galaxy system located 300 million light years away in the constellation Aquarius. It was discovered by William Herschel on September 20, 1784. [3] The total infrared luminosity is 10 11.33 L ☉, and thus it is categorised as a luminous infrared galaxy. [4] One of the galaxies hosts a type 2 Seyfert nucleus. [5]

The small group of galaxies around NGC 7585 (NGC 7576 and NGC 7592) in Aquarius were all discovered by William Herschel. He found NGC 7585 and NGC 7592 in September 1784 but NGC 7576 had to wait until the following year in October 1785 to be picked up, although Herschel did not spot that NGC 7592 was a double galaxy.

NGC 7592 is a Spiral Galaxy located in the constellation of Aquarius in the equatorial region. NGC 7592 is called NGC 7592 in the New General Catalogue (NGC). This catalogue is a list of deep space objects compiled by John Louis Emil Dreyer in 1888 to …

The complex nature of the Seyfert galaxy NGC 7592 Long slit spectra of NGC 7592 were taken on Sep. 26 to 30, 1989 at the 1.52 cm European Southern Observatory (ESO) telescope, equipped with a Boller and Chivens spectrograph and an RCA High Resolution charge coupled device (CCD) camera. The problem of the nature of Region C is addressed at first.

2024年2月4日 · Based on a recessional velocity of 1610 km/sec, NGC 7552 is about 75 million light years away, in reasonable agreement with redshift-independent distance estimates of 55 to 70 million light years. Given that and its apparent size of 3.4 by 2.7 arcmin, it is about 75 thousand light years across.

In this paper we present a detailed analysis of the physical conditions and of the kinematical and dynamical properties of the system of interacting galaxies NGC 7592, the western component of which shows signs of Seyfert activity.

Abstract: We performed a tridimensional spectroscopic study of NGC 7592, an infrared-luminous interacting system of three galaxies, one of which contains a Seyfert 2 nucleus. Narrow-band images of $\rm{H}\alpha$ and [O iii] were obtained using an imaging Fabry–Perot interferometer with a tunable filter.

NGC 7592A is a Galaxy in the Aquarius constellation. NGC 7592A is situated close to the celestial equator and, as such, it is at least partly visible from both hemispheres in certain times of the year. Given its visual magnitude of 15, NGC 7592A is visible with the help of a telescope having an aperture of 20 inches (500mm) or more.

2002年6月25日 · We performed a tridimensional spectroscopic study of NGC 7592, an infrared-luminous interacting system of three galaxies, one of which contains a Seyfert 2 nucleus. Narrow-band images of H α and [O iii] were obtained using an imaging Fabry–Perot interferometer with a …

The relation between mergers and AGN activity. Results from radio galaxy and luminous infrared galaxy studies There is morphological evidence that the activity in powerful radiogalaxies could be triggered by mergers and galaxy interactions.