Monitoring Water Masers in Star-Forming Regions
Monitoring Water Masers in Star-Forming Regions
复制标题
监测恒星形成区域的水脉泽
DOI：
10.1007/s10509-005-3673-2
复制
发表时间：
2004
影响因子：
1.9
通讯作者：
R. Valdettaro
中科院分区：
文献类型：
--
作者：
J. Brand;R. Cesaroni;G. Comoretto;M. Felli;F. Palagi;F. Palla;R. Valdettaro
An overview is given of the analysis of more than a decade of H2O maser data from our monitoring program. We find the maser emission to generally depend on the luminosity of the YSO as well as on the geometry of the SFR. There appears to be a threshold luminosity of a few times 104L⊙ above and below which we find different maser characteristics.
