We apply Dicke’s theory of superradiance (introduced in 1954) to the 6.7-GHz methanol and 22-GHz water spectral lines, often detected in molecular clouds as signposts for the early stages of the star formation process. We suggest that superradiance, characterized by burst-like features taking place over a wide range of time scales, may provide a natural explanation for the recent observations of periodic and seemingly alternating methanol and water maser flares in G107.298+5.639. Although these observations would be very difficult to explain within the context of maser theory, we show that these flares may result from simultaneously initiated 6.7-GHz methanol and 22-GHz water superradiant bursts operating on different time scales, thus prov...
We report on the detection of bursts of 6.7 GHz methanol maser emission in a high-mass star-forming ...
We present detailed modeling of periodic flaring events in the 6.7 GHz and 12.2 GHz methanol lines a...
We report the detection of a new class I methanol maser candidate from the 52-41 E transition (266.8...
We present new evidence for superradiance (SR) in the methanol 6.7 GHz spectral line for three diffe...
We apply the concept of superradiance that was introduced by Dicke in 1954 to the OH molecule 1612 M...
It is generally assumed that in the interstellar medium much of the emission emanating from atomic a...
Context: Periodic flares of maser emission are thought to be induced either by variations of the see...
Discovery of periodic maser emission was an unexpected result from monitoring observations of methan...
Context.High-mass young stellar objects (HMYSOs) can undergo accretion episodes that stron...
Since the discovery of periodic class II methanol masers at 6.7 and 12.2 GHz associated with high-ma...
We report the first detection of isotopic methanol (13CH3OH) maser emission in interstellar space. T...
We report the detection of new 12.178, 12.229, 20.347, and 23.121 GHz methanol masers in the massive...
Context. Recent studies have shown that 6.7 GHz methanol maser flares can be a powerful tool for ver...
The source G25.65+1.05 (RAFGL7009S, IRAS 18316-0602) is the least studied of the three regions of ma...
We have performed a molecular line search toward the flaring 6.7-GHz masers G24.33+0.13 and G359.62-...
We report on the detection of bursts of 6.7 GHz methanol maser emission in a high-mass star-forming ...
We present detailed modeling of periodic flaring events in the 6.7 GHz and 12.2 GHz methanol lines a...
We report the detection of a new class I methanol maser candidate from the 52-41 E transition (266.8...
We present new evidence for superradiance (SR) in the methanol 6.7 GHz spectral line for three diffe...
We apply the concept of superradiance that was introduced by Dicke in 1954 to the OH molecule 1612 M...
It is generally assumed that in the interstellar medium much of the emission emanating from atomic a...
Context: Periodic flares of maser emission are thought to be induced either by variations of the see...
Discovery of periodic maser emission was an unexpected result from monitoring observations of methan...
Context.High-mass young stellar objects (HMYSOs) can undergo accretion episodes that stron...
Since the discovery of periodic class II methanol masers at 6.7 and 12.2 GHz associated with high-ma...
We report the first detection of isotopic methanol (13CH3OH) maser emission in interstellar space. T...
We report the detection of new 12.178, 12.229, 20.347, and 23.121 GHz methanol masers in the massive...
Context. Recent studies have shown that 6.7 GHz methanol maser flares can be a powerful tool for ver...
The source G25.65+1.05 (RAFGL7009S, IRAS 18316-0602) is the least studied of the three regions of ma...
We have performed a molecular line search toward the flaring 6.7-GHz masers G24.33+0.13 and G359.62-...
We report on the detection of bursts of 6.7 GHz methanol maser emission in a high-mass star-forming ...
We present detailed modeling of periodic flaring events in the 6.7 GHz and 12.2 GHz methanol lines a...
We report the detection of a new class I methanol maser candidate from the 52-41 E transition (266.8...