IRAS 14070 + 0525 - an OH gigamaser at z = 0.265

Details IRAS 14070 + 0525 - an OH gigamaser at z = 0.265 IRAS 14070 + 0525 - an OH gigamaser at z = 0.265

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...396l..99b&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 396, no. 2, Sept. 10, 1992, p. L99-L102.

Astronomy and Astrophysics

Astronomy

28

Galaxies, Hydroxyl Radicals, Infrared Sources (Astronomy), Interstellar Masers, Galactic Evolution, Galactic Nuclei, Interacting Galaxies, Luminosity

Scientific paper

OH gigamaser emission has been detected in the luminous FIR galaxy IRAS 14070 + 0525 at a redshift of 0.265. The FIR luminosity of IRAS 14070 + 0525 is 10 exp 12.5 solar luminosities. The OH line luminosity is 14,000 solar luminosities, making it the most luminous known OH emitter. The OH line emission covers a velocity range of approximately 2400 km/s. Two distinct components in the OH emission reveal a powerful outflow component and/or the interactive nature of the system.

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