Monitoring Water Masers in Star-Forming Regions

被引:0
|
作者
J. Brand
R. Cesaroni
G. Comoretto
M. Felli
F. Palagi
F. Palla
R. Valdettaro
机构
[1] Istituto di Radioastronomia,
[2] CNR,undefined
[3] INAF-Osservatorio Astrofisico di Arcetri,undefined
[4] Instituto di Radioastronomia,undefined
[5] CNR,undefined
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water masers; monitoring;
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摘要
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.
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页码:133 / 141
页数:8
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