Monitoring water masers in star-forming regions

Details Monitoring water masers in star-forming regions Monitoring water masers in star-forming regions

2004-07-12

arxiv.org/abs/astro-ph/0407217v1

Astrophys.Space Sci. 295 (2005) 133-141

Astronomy and Astrophysics

Astrophysics

9 pages, 1 table, 11 figures. Accepted for publ. in Ap&SpSci. Refereed contribution to "Dense Molecular Gas around Protostars

Scientific paper

10.1007/s10509-005-3673-2

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 10**4 Lsol above and below which we
find different maser characteristics.

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