A survey of Class II methanol masers at 6.7 GHz was made in the Northern hemisphere with the 32-m Medicina radio telescope. 42 objects were detected, 20 of them are new detections at 6.7 GHz. Our results show that the detection rate of 6.7 GHz masers toward the inner part of the Galaxy is higher than in other directions. It is confirmed that most of the methanol masers are associated with faint compact HII regions. The 6.7 GHz methanol masers show large velocity dispersion and large velocity offset from the velocity of parent molecular clouds
Abstract The Purple Mountain Observatory 13.7 m radio telescope has been used to search for 95 GHz (...
Context. Maser lines from different molecular species, including water, hydroxyl, and meth...
Sorry, the full text of this article is not available here. Please click on the alternative location...
A survey of Class II methanol masers at 6.7 GHz was made in the Northern hemisphere with the 32-m Me...
Methanol masers are often detected in regions of intense star formation. Several studies in the las...
Methanol masers are often detected in regions of intense star formation. Several studies in the last...
The 6.7 GHz transition of methanol is the strongest of methanol masers, and is the second strongest ...
Restricted AccessWe present initial results of a blind survey for 6.7 GHz methanol masers that is be...
The 6.7 GHz transition of methanol is the strongest of methanol masers, and is the second strongest ...
The Methanol Multibeam survey has produced the largest and most complete census of methanol and exci...
The Methanol Multibeam survey has produced the largest and most complete census of methanol and exci...
We present the results of a high sensitivity survey for 6.7 GHz methanol masers towards 22 GHz water...
The Purple Mountain Observatory 13.7 m radio telescope has been used to search for 95 GHz (8(0)-7(1)...
The Purple Mountain Observatory 13.7 m radio telescope has been used to search for 95 GHz (80–71A+) ...
In 1991 maser emission from the 51-60 A+ transition of CH3OH at a frequency of 6.7 GHz was discover...
Abstract The Purple Mountain Observatory 13.7 m radio telescope has been used to search for 95 GHz (...
Context. Maser lines from different molecular species, including water, hydroxyl, and meth...
Sorry, the full text of this article is not available here. Please click on the alternative location...
A survey of Class II methanol masers at 6.7 GHz was made in the Northern hemisphere with the 32-m Me...
Methanol masers are often detected in regions of intense star formation. Several studies in the las...
Methanol masers are often detected in regions of intense star formation. Several studies in the last...
The 6.7 GHz transition of methanol is the strongest of methanol masers, and is the second strongest ...
Restricted AccessWe present initial results of a blind survey for 6.7 GHz methanol masers that is be...
The 6.7 GHz transition of methanol is the strongest of methanol masers, and is the second strongest ...
The Methanol Multibeam survey has produced the largest and most complete census of methanol and exci...
The Methanol Multibeam survey has produced the largest and most complete census of methanol and exci...
We present the results of a high sensitivity survey for 6.7 GHz methanol masers towards 22 GHz water...
The Purple Mountain Observatory 13.7 m radio telescope has been used to search for 95 GHz (8(0)-7(1)...
The Purple Mountain Observatory 13.7 m radio telescope has been used to search for 95 GHz (80–71A+) ...
In 1991 maser emission from the 51-60 A+ transition of CH3OH at a frequency of 6.7 GHz was discover...
Abstract The Purple Mountain Observatory 13.7 m radio telescope has been used to search for 95 GHz (...
Context. Maser lines from different molecular species, including water, hydroxyl, and meth...
Sorry, the full text of this article is not available here. Please click on the alternative location...