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Messier 82 (also known as NGC 3034, Cigar Galaxy or M82) is a starburst galaxy approximately 12 million light-years away in the constellation Ursa Major. It is the second-largest member of the M81 Group , with the D 25 isophotal diameter of 12.52 kiloparsecs (40,800 light-years ).
It also contains regions of ionized hydrogen and is a starburst galaxy. NGC 3049 is also a field galaxy, that is to say it does not belong to a cluster or group and is therefore gravitationally isolated. [2] NGC 3049 is a galaxy whose core shines in the field of ultraviolet. It is listed in the Markarian catalog under the reference Mrk 710 (MK ...
SDSS J113706.18-033737.1 (PGC 125758) is a dwarf starburst galaxy with a mass of 100 times the mass of the sun. This galaxy is located 395 million light years away from earth. It is currently undergoing a burst of stellar formation forming 0.5 solar masses a year. [2] [3]
The Antennae Galaxies are an example of a starburst galaxy occurring from the collision of NGC 4038/NGC 4039. Credit: NASA/ESA. A starburst galaxy is one undergoing an exceptionally high rate of star formation, as compared to the long-term average rate of star formation in the galaxy, or the star formation rate observed in most other galaxies.
NGC 3125 is a large starburst galaxy in the constellation Antlia.It is located approximately 50 million light-years away from Earth.Starburst galaxies are galaxies in which unusually high numbers of new stars are forming, springing to life within intensely hot clouds of gas.
NGC 3310 is a grand design spiral galaxy in the constellation Ursa Major.It is a starburst galaxy and it is likely that NGC 3310 collided with one of its satellite galaxies about 100 million years ago, triggering widespread star formation.
HXMM01, known more formally as 1HERMES S250 J022016.5−060143, is a starburst galaxy [2] located in the northwestern portion of the constellation Cetus. [note 1] Discovered in 2013 by a team at the University of California, Irvine, it was discovered that HXMM01 is actually still forming from its two parent galaxies as part of the "brightest, most luminous and most gas-rich submillimeter ...
Hen 2-10 is a starburst galaxy featuring at least two star-forming regions near the center of the galaxy. [6] These regions feature a variety of different substances, and multiple super star clusters. A study of some of these SSCs estimates their age to be between 4 and 5 megayears. [7]