A new pumping mechanism - methanol masers without population inversion is presented in this paper. It can be used to explain the formation of a series of J(0) --> J(-)1 E methanol masers, while the 2(1) --> 3(0) A(+) methanol masers are regarded as a driving coherent micrwave field. In the new mechanism, the intensities of J(0) - J(-)1 E methanol masers are increased with the decreasing transition frequencies (or with rotational number J, approximately). These results agree with Slysh et al. (1995) and Slysh et al. (1999) J less than or equal to 5 observations for G3345.01+1.79 and W48, in which both J(0) --> J(-)1 E and 2(1) --> 3(0) A(+) methanol masers are detected coincidentally. Other astronomical conditions, such as magnet...
General characteristics of methanol (CH3OH) maser emission are summarized. It is shown that methanol...
We report the detection of a new class I methanol maser candidate from the 52-41 E transition (266.8...
We present the unambiguous discovery of six new class II methanol maser transitions, three of which ...
$^{a}$ G. Prasad, and G. Agarwal, Optics Comm. 86, 409 (1991)Author Institution: Department of Physi...
It is recognized that the interstellar methanol-107 GHz masers and OH-4.765 GHz masers towards Class...
Abstract It is recognized that the interstellar methanol-107GHz masers and OH-4.765GHz masers toward...
We review properties of all known collisionally pumped (class I) methanol maser series based on obse...
We review properties of all known collisionally pumped (class I) methanol maser series based on obse...
Context. Class I methanol masers are thought to be tracers of interstellar shock waves. However, the...
Context. Class I methanol masers are thought to be tracers of interstellar shock waves. However, the...
As first realised in the late 1980s, methanol masers come in two varieties, termed Class I and Class...
Model spectra are presented for Class II methanol masers under a variety of conditions. The model is...
We have used the Swedish ESO Submillimetre Telescope (SEST) to search for new classII methanol maser...
A number of mechanisms for understanding the periodic class II methanol masers associated with some ...
Context. Astronomical masers have been effective tools in the study of magnetic fields for years. Ob...
General characteristics of methanol (CH3OH) maser emission are summarized. It is shown that methanol...
We report the detection of a new class I methanol maser candidate from the 52-41 E transition (266.8...
We present the unambiguous discovery of six new class II methanol maser transitions, three of which ...
$^{a}$ G. Prasad, and G. Agarwal, Optics Comm. 86, 409 (1991)Author Institution: Department of Physi...
It is recognized that the interstellar methanol-107 GHz masers and OH-4.765 GHz masers towards Class...
Abstract It is recognized that the interstellar methanol-107GHz masers and OH-4.765GHz masers toward...
We review properties of all known collisionally pumped (class I) methanol maser series based on obse...
We review properties of all known collisionally pumped (class I) methanol maser series based on obse...
Context. Class I methanol masers are thought to be tracers of interstellar shock waves. However, the...
Context. Class I methanol masers are thought to be tracers of interstellar shock waves. However, the...
As first realised in the late 1980s, methanol masers come in two varieties, termed Class I and Class...
Model spectra are presented for Class II methanol masers under a variety of conditions. The model is...
We have used the Swedish ESO Submillimetre Telescope (SEST) to search for new classII methanol maser...
A number of mechanisms for understanding the periodic class II methanol masers associated with some ...
Context. Astronomical masers have been effective tools in the study of magnetic fields for years. Ob...
General characteristics of methanol (CH3OH) maser emission are summarized. It is shown that methanol...
We report the detection of a new class I methanol maser candidate from the 52-41 E transition (266.8...
We present the unambiguous discovery of six new class II methanol maser transitions, three of which ...