As first realised in the late 1980s, methanol masers come in two varieties, termed Class I and Class II. While Class II masers had observationally been extensively studied in the past, until recently relatively little attention was paid to Class I methanol masers due to their low luminosities compared to other maser transitions. In this review, we will focus on the recent progress in our understanding of Class I methanol masers both from an observational and from a theoretical point of view
The class II masers of methanol are associated with the early stages of formation of high-mass stars...
The Australia Telescope Compact Array has been used to make the first extensive search for the class...
A new pumping mechanism - methanol masers without population inversion is presented in this paper. I...
We review properties of all known collisionally pumped (class I) methanol maser series based on obse...
The class II masers of methanol are associated with the early stages of formation of high-mass stars...
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...
General characteristics of methanol (CH3OH) maser emission are summarized. It is shown that methanol...
We review properties of all known collisionally pumped (class I) methanol maser series based on obse...
Model spectra are presented for Class II methanol masers under a variety of conditions. The model is...
We have used the Australia Telescope Compact Array (ATCA) to make the first high-resolution observat...
We report the detection of a new class I methanol maser candidate from the 52-41 E transition (266.8...
We report the detection of a new class I methanol maser candidate from the 52-41 E transition (266.8...
We report the detection with the ATCA of 6.7 GHz methanol emission towards OMC-1. The source has a s...
We have used the Swedish ESO Submillimetre Telescope (SEST) to search for new classII methanol maser...
The class II masers of methanol are associated with the early stages of formation of high-mass stars...
The Australia Telescope Compact Array has been used to make the first extensive search for the class...
A new pumping mechanism - methanol masers without population inversion is presented in this paper. I...
We review properties of all known collisionally pumped (class I) methanol maser series based on obse...
The class II masers of methanol are associated with the early stages of formation of high-mass stars...
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...
General characteristics of methanol (CH3OH) maser emission are summarized. It is shown that methanol...
We review properties of all known collisionally pumped (class I) methanol maser series based on obse...
Model spectra are presented for Class II methanol masers under a variety of conditions. The model is...
We have used the Australia Telescope Compact Array (ATCA) to make the first high-resolution observat...
We report the detection of a new class I methanol maser candidate from the 52-41 E transition (266.8...
We report the detection of a new class I methanol maser candidate from the 52-41 E transition (266.8...
We report the detection with the ATCA of 6.7 GHz methanol emission towards OMC-1. The source has a s...
We have used the Swedish ESO Submillimetre Telescope (SEST) to search for new classII methanol maser...
The class II masers of methanol are associated with the early stages of formation of high-mass stars...
The Australia Telescope Compact Array has been used to make the first extensive search for the class...
A new pumping mechanism - methanol masers without population inversion is presented in this paper. I...