Astrophysical Masers pp 303-306 | Cite as
Water maser bursts in W49M (1989–92)
11. Variability
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Abstract
After an extensive monitoring program of the water vapour emission originated from W49N we were able to detect very strong eruptions at +28 km/s, −61 km/s and −27 km/s. Here we present the results of the monitoring of these explosions and discuss the possible correlated variability of the events recorded at +28 km/s with one of them, not so intense, that appeared at +62 km/s.
Keywords
Antenna Temperature Solar Luminosity Strong Flare Strong Eruption Halfpower Beamwidth
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© Springer-Verlag 1993