The brightest OH maser in the sky: a flare of emission in W75 N

Abstract

A flare of maser radio emission in the OH-line 1665 MHz has been discovered in the star forming region W75 N in 2003, with the flux density of about 1000 Jy. At the time it was the strongest OH maser detected during the whole history of observations since the discovery of cosmic masers in 1965. The flare emission is linearly polarized with a degree of polarization near 100%. A weaker flare with a flux of 145 Jy was observed in this source in 2000 - 2001, which was probably a precursor of the powerful flare. Intensity of two other spectral features has decreased after beginning of the flare. Such variation of the intensity of maser condensation emission (increasing of one and decreasing of the other) can be explained by passing of the magneto hydrodynamic shock across regions of enhanced gas concentration.

arXiv comment9 pages with 2 figures, accepted for publication in Astronomy Letters

References in corpus (2)

• The Nature of the Massive Young Stars in W75 N
• Total linear polarization in the OH maser W75N: VLBA polarization structure

Cited by in corpus (9)

• The structure of the magnetic field in the massive star-forming region W75N
• Methanol masers probing the ordered magnetic field of W75N
• Structure of W3(OH) from Very High Spectral Resolution Observations of 5 Centimeter OH Masers
• A bright radio HH object with large proper motions in the massive star-forming region W75N
• Strong magnetic field in W75N OH maser flare
• Large Magnetic Fields and Motions of OH Masers in W75 N
• Flares and Proper Motions of Ground-State OH Masers in W75N
• Monitoring of the polarized $H_{2}O$ maser emission around the massive protostars W75N(B)-VLA1 and W75N(B)-VLA2
• Masers and star formation