Acronym/Abbreviation meaning of ULIRG (Chemistry)

The acronym ULIRG(Chemistry) means : Ultraluminous Infrared Galaxy

Acronyms, abbreviations and meanings similar to ULIRG

Ultraluminous Infrared Galaxy

Ultra Luminous Infrared Galaxy

Famous / Popular results for ULIRG

Luminous infrared galaxy

Galaxies with luminosities above 1012 L☉ are ultraluminous infrared galaxies (ULIRGs). Galaxies exceeding 1013 L☉ are characterised as hyper-luminous infrared

NGC 6240

NGC 6240 is a nearby ultraluminous infrared galaxy (ULIRG) in the constellation Ophiuchus. The galaxy is the remnant of a merger between two smaller galaxies

Starburst galaxy

associated with ULIRGs. It is not known for sure that the UV radiation is produced purely by star-formation, and some astronomers believe ULIRGs to be powered

Arp 220

Peculiar Galaxies. Arp 220 is the closest Ultraluminous Infrared Galaxy (ULIRG) to Earth. Its energy output was discovered by IRAS to be dominated by the

APM 08279+5255

and by the newly forming stars. APM is an ultra-luminous infrared galaxy (ULIRG). Its high redshift shifts the far-infrared spectrum into millimeter wavelengths

List of galaxies

"Optical spectroscopy of Arp220: the star formation history of the closest ULIRG". Monthly Notices of the Royal Astronomical Society. 384 (3): 875–885. arXiv:0711

Galaxy filament

Springer-Verlag Berlin Heidelberg, 2008, p. 358 "Ultraviolet-Bright, High-Redshift ULIRGS" 00/2008 Bibcode: 2008ralc.conf..358W Zitrin, A.; Brosch, N. (2008). "The

Seyfert galaxy

Seyfert galaxy NGC 6240, also classified as an ultraluminous infrared galaxy (ULIRG) NGC 6251, the X-ray brightest low-excitation radio galaxy in the 3CRR catalog

Megamaser

likely to host hydroxyl megamasers, as are ULIRGs, with LFIR > 1012 L☉. At least one out of three ULIRGs hosts an hydroxyl megamaser, as compared with

FSC15307+3253

FSC15307+3253 (or IRAS F15307+3252) is an ultraluminous infrared galaxy (ULIRG), with a luminosity between 8 and 1000 µm of approximately 2×1013 L⊙, possibly

Luminous infrared galaxy

Galaxies with luminosities above 1012 L☉ are ultraluminous infrared galaxies (ULIRGs). Galaxies exceeding 1013 L☉ are characterised as hyper-luminous infrared

NGC 6240

NGC 6240 is a nearby ultraluminous infrared galaxy (ULIRG) in the constellation Ophiuchus. The galaxy is the remnant of a merger between two smaller galaxies

Starburst galaxy

associated with ULIRGs. It is not known for sure that the UV radiation is produced purely by star-formation, and some astronomers believe ULIRGs to be powered

Arp 220

Peculiar Galaxies. Arp 220 is the closest Ultraluminous Infrared Galaxy (ULIRG) to Earth. Its energy output was discovered by IRAS to be dominated by the

APM 08279+5255

and by the newly forming stars. APM is an ultra-luminous infrared galaxy (ULIRG). Its high redshift shifts the far-infrared spectrum into millimeter wavelengths

List of galaxies

"Optical spectroscopy of Arp220: the star formation history of the closest ULIRG". Monthly Notices of the Royal Astronomical Society. 384 (3): 875–885. arXiv:0711

Galaxy filament

Springer-Verlag Berlin Heidelberg, 2008, p. 358 "Ultraviolet-Bright, High-Redshift ULIRGS" 00/2008 Bibcode: 2008ralc.conf..358W Zitrin, A.; Brosch, N. (2008). "The

Seyfert galaxy

Seyfert galaxy NGC 6240, also classified as an ultraluminous infrared galaxy (ULIRG) NGC 6251, the X-ray brightest low-excitation radio galaxy in the 3CRR catalog

Megamaser

likely to host hydroxyl megamasers, as are ULIRGs, with LFIR > 1012 L☉. At least one out of three ULIRGs hosts an hydroxyl megamaser, as compared with

FSC15307+3253

FSC15307+3253 (or IRAS F15307+3252) is an ultraluminous infrared galaxy (ULIRG), with a luminosity between 8 and 1000 µm of approximately 2×1013 L⊙, possibly

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