Elliptical Galaxy M59
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Messier 59 or M59, also known as NGC 4621, is an elliptical galaxy in the equatorial
constellation A constellation is an area on the celestial sphere in which a group of visible stars forms Asterism (astronomy), a perceived pattern or outline, typically representing an animal, mythological subject, or inanimate object. The origins of the e ...
of Virgo. It is a member of the Virgo Cluster, with the nearest fellow member away and around 5 magnitudes fainter. The nearest cluster member of comparable brightness is the lenticular galaxy
NGC 4638 NGC 4638 is an edge-on lenticular galaxy located about 50 million light-years away in the constellation Virgo. NGC 4638 was discovered by astronomer William Herschel on March 15, 1784. The galaxy is a member of the Virgo Cluster. Structure ...
, which is around away. It and the angularly nearby elliptical galaxy Messier 60 were both discovered by Johann Gottfried Koehler in April 1779 when observing comet seeming close by. Charles Messier listed both in the Messier Catalogue about three days after Koehler's discovery. This is an elliptical galaxy of type E5 with a position angle of 163.3°, indicating the overall shape shows a flattening of 50%. However, isophotes for this galaxy deviate from a perfect ellipticity, showing pointed shapes instead. These can be decomposed mathematically into a three component model, with each part having a different eccentricity. The main elliptical component appears to be superimposed upon a flatter, disk-like feature, with the entirety embedded within a circular halo. The luminosity contribution of the components is 62% for the pure elliptical part, 22% for the halo, and the remainder coming from the disk. The light ratio of the disk to the main elliptical body is 0.25, whereas it is typically closer to 0.5 in a lenticular galaxy. The core contains a supermassive black hole (SMBH), with a mass that has been estimated to be 270 million times the
mass of the Sun The solar mass () is a standard unit of mass in astronomy, equal to approximately . It is often used to indicate the masses of other stars, as well as stellar clusters, nebulae, galaxies and black holes. It is approximately equal to the mass ...
, and counter-rotates with respect of the rest of the galaxy, being bluer. The SMBH is quiescent, but is detectable as an X-ray and radio source that indicates an outflow. The nucleus contains an embedded stellar disk that is bluer (younger) than the bulge region, with a blue component stretching along a position angle of around 150°. This extended disk feature may be the result of a galactic merger followed by a
starburst MicroPro International Corporation was an American software company founded in 1978 in San Rafael, California. They are best known as the publisher of WordStar, a popular early word processor for personal computers. History Founding and early su ...
event. Messier 59 is very rich in globular clusters, with a population of them that has been estimated to be around 2,200. It has two satellites, the ultra compact dwarf galaxy M59-UCD3 and M59cO, which is a rare example of a galaxy in between
compact ellipticals Compact as used in politics may refer broadly to a pact or treaty; in more specific cases it may refer to: * Interstate compact * Blood compact, an ancient ritual of the Philippines * Compact government, a type of colonial rule utilized in British ...
such as Messier 32 and ultra compact dwarfs. One supernova (1939B) has been recorded in M59; it reached a peak magnitude of 11.9. The region where this supernova occurred shows no trace of star formation, which suggests this was a type Ia supernova.


See also

* List of Messier objects


References


External links


Elliptical Galaxy M59 @ SEDS Messier pages
* {{DEFAULTSORT:Messier 59 Messier 059 Messier 059 Messier 059 059 Messier 059 07858 42628 Astronomical objects discovered in 1779