ESO 383-76
ESO 383-76 is an elongated, X-ray luminous supergiant elliptical galaxy, residing as the dominant, brightest cluster galaxy of the Abell 3571 galaxy cluster, the sixth-brightest in the sky at X-ray wavelengths. It is located at the distance of from Earth, and is possibly a member of the large Shapley Supercluster. With a diameter of about, it is one of the largest galaxies known. It also contains a supermassive black hole, one of the most massive known with mass estimates varying from to.
Observation history
The first known observation of the galaxy was during the creation of the Morphological Catalogue of Galaxies by Boris Vorontsov-Velyaminov and V.P. Harkipova in 1974, with the catalogue entry MCG-05-33-002. The galaxy was also observed around this time by the ESO Sky Survey Atlas, a large-scale survey of the Southern Sky conducted using the 1-metre Schmidt telescope in La Silla Observatory. In 1982, the ESO/Uppsala Catalogue then lists the galaxy in its current designation form – ESO 383-G 076, indicating both its field number, classification, and its numerical identifier in its field. The galaxy, at this point, was nothing more than just an obscure catalogue entry.O.G. Richter in 1984 then observed the galaxy during a redshift survey of the ESO/SRC Survey Fields 444 and 445 of the Klemola 27 group. The group consists of prominent galaxies such as the namesake IC 4329 – another massive supergiant elliptical that is also an extreme Seyfert galaxy, and NGC 5291 – a disturbed interacting galaxy pair. ESO 383-76, initially thought to be a member of this group, was listed as the 442nd galaxy in Richter's table entry and has been given the morphology E/S0. The galaxy has also been included in the Southern Galaxy Catalogue, containing nearly 5,000 galaxies, compiled in 1985 by the husband-and-wife astrophysicists Gérard and Antoinette de Vaucouleurs, along with H.G. Corwin Jr.
ESO 383-76 would be additionally recorded in many subsequent galaxy surveys, such as the survey of the Hydra–Centaurus Supercluster by L.N. da Costa et al in 1986, and moreover a photometric catalogue by Lauberts and Valentijn in 1989 that made the first angular diameter measurements of the galaxy. This includes the D25 and D25.5 B-band isophotes, as well as the 50% total light emission and variations of it. A.P. Fairall et al would further incorporate the galaxy in their wide-scale survey of the Hydra-Centaurus Supercluster in 1989. It was additionally included in many other surveys due to its location in the sky in the rich Centaurus region and the wide-scale research of extragalactic objects near the Milky Way plane by the last decade of the 20th century. The galaxy has additionally been catalogued by Alan Dressler in 1991 during an analysis of velocities of 1,314 galaxies near the Milky Way galactic plane region – allowing to pinpoint the location and verify the existence of the Great Attractor.
Description
ESO 383-76 is a supergiant elliptical galaxy of an advanced Hubble morphology, with its major axis being more than twice the length of its minor axis. The galaxy is a very luminous source of X-rays, and is the sixth-brightest X-ray source in the sky.In an analysis of the cluster A3571 by H. Quintana and R. de Souza in 1994, ESO 383-76 has been noted to have a very elongated shape with a diffuse halo extending throughout the cluster, suggesting that the galaxy had formed very early during the formation of Abell 3571 and it retains the original imprint of its collapsing cloud. The mass of the core region, which also includes the galaxy, is on the order of.
Size
There are various methods used in astronomy in defining the size of a galaxy, and each of them can yield different results with respect to the other. This is usually affected by exposure time, the wavelength used, and the instrument being used.One method that is commonly used in the astronomical literature is the galaxy effective radius where 50% of the total galaxy's light was emitted; variations of 60%, 70%, and 90% are also used. An estimation of the galaxy's size by the ESO/Uppsala catalogue's broad-band photographic plates in 1989 using the 90% total light definition yield a very large apparent diameter of 555.9 arcseconds, which using the currently accepted distance to the galaxy yield a diameter of. This makes it one of the largest physical diameter measurements of any galaxy known – 20 times that of the Milky Way's diameter, and 3.5 times that of the maximum estimated diameter of IC 1101.
Alternative measurements from the same study using other methods yield diameters as small as, with various estimates in between depending on the measurement. In a study in 1994, the halo of the galaxy has a diameter of about. The paper states that this is on the scale of the distance between the Milky Way and Andromeda galaxies. The halo extends throughout a large part of Abell 3571.