The Medicina survey of methanol masers at 6.7 GHz

被引:87
作者
Slysh, VI
Val'tts, IE
Kalenskii, SV
Voronkov, MA
Palagi, F
Tofani, G
Catarzi, M
机构
[1] CNR, CAISMI, I-50125 Florence, Italy
[2] PN Lebedev Phys Inst, Ctr Astro Space, Moscow 117810, Russia
[3] Moscow MV Lomonosov State Univ, Fac Phys, Dept Astron, Moscow 119899, Russia
[4] Osservatorio Astrofis Arcetri, I-50125 Florence, Italy
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1999年 / 134卷 / 01期
关键词
masers; ISM : molecules; HII regions; radio lines : ISM;
D O I
10.1051/aas:1999127
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 tl-lan in other directions. It is confirmed tl-lat 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.
引用
收藏
页码:115 / 128
页数:14
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