Exploring OH Megamasers

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چکیده

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Zeeman splitting in OH megamasers

We detected significant Zeeman splitting in the 1667MHz OH megamaser emission from four ultraluminous galaxies. These detections, in addition to being the first extragalactic detection of the Zeeman effect in an emission line, suggest that OH megamasers are excellent extragalactic magnetometers.

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A Dense Gas Trigger for Oh Megamasers

HCN and CO line diagnostics provide new insight into the OH megamaser (OHM) phenomenon, suggesting a dense gas trigger for OHMs. We identify three physical properties that differentiate OHM hosts from other starburst galaxies: (1) OHMs have the highest mean molecular gas densities among starburst galaxies; nearly all OHM hosts have n̄(H2) = 103–104 cm−3 (OH line-emitting clouds likely have n(H2)...

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Extragalactic Zeeman Detections in Oh Megamasers

We have measured the Zeeman splitting of OH megamaser emission at 1667 MHz from five (ultra)luminous infrared galaxies ([U]LIRGs) using the 305 m Arecibo telescope and the 100 m Green Bank Telescope. Five of eight targeted galaxies show significant Zeeman-splitting detections, with 14 individual masing components detected and line-of-sight magnetic field strengths ranging from ≃ 0.5 − 18 mG. Th...

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OH megamasers , starburst and AGN activity in Markarian 231

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A Search for OH Megamasers at z> 0.1: Preliminary Results

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ژورنال

عنوان ژورنال: Highlights of Astronomy

سال: 1998

ISSN: 1539-2996

DOI: 10.1017/s1539299600019249