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Facing and Overcoming Sensitivity Challenges in Biomolecular NMR Spectroscopy. [PDF]
Ardenkjaer-Larsen JH +18 more
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Efficient detection of water masers
Nature, 1988During the past 15 years almost 190 natural sources of 22 GHz water maser emission have been found in the dusty circumstellar shells of late-type stars undergoing mass-loss. Numbered among these sources are ∼75% of the Mira variables within 400 pc of the Sun1, although only 34% of Miras in general are associated with OH masers2.
B. M. Lewis, D. Engels
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Modelling interstellar water masers
Astrophysics and Space Science, 1995Radiative transfer calculations for interstellar H2O have been performed using accelerated A-iteration (ALI) techniques. The results show strong maser action from known maser transitions, as well as predicting new strong maser transitions for ν > 1.5 THz. © 1995 Kluwer Academic Publishers.
Yates, JA, Gray, MD, Field, D
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Water masers in red supergiants
Astronomical & Astrophysical Transactions, 2006Results of long-term monitoring of circumstellar water maser sources in red supergiants are reviewed. The observations were carried out in 1980–2006 on the RT-22 radio telescope at Pushchino Radio Astronomy Observatory. We discuss the results for the semiregular variable M-supergiant VX Sgr and non-variable M-supergiant IRC–10414.
M. I. Pashchenko +3 more
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Interstellar hydroxyl and water masers and formaldehyde masers and dasars
Reports on Progress in Physics, 1974A review of the observational data on anomalous emission by OH, H2O and H2CO molecules and on anomalous absorption by H2CO molecules. Various theories advanced to account for these data and some models of a few particular sources are discussed.
D ter Haar, M A Pelling
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1993
The excitation of maser emission in millimeter and submillimeter transitions of interstellar and circumstellar water is considered. Using an escape probability method, the equilibrium populations in 349 rotational states of both ortho- and para-water have been determined under varying conditions of gas temperature, density, water abundance and ...
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The excitation of maser emission in millimeter and submillimeter transitions of interstellar and circumstellar water is considered. Using an escape probability method, the equilibrium populations in 349 rotational states of both ortho- and para-water have been determined under varying conditions of gas temperature, density, water abundance and ...
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