... OF THE GALACTICPLANE BETWEEN . l = 343^o AND l = 19^o AND |b| < 5.5^o AT 0.96, 3.9 AND 11.2 GHZ . S.A. TRUSHKIN . REFERENCES. ... The three-frequency radio survey of the Galacticplane has been made at 0.96, 3.9 and 11.2 GHz with the RATAN-600 radio ...
... with the MPFS and SCORPIO spectrographs indicates that we are dealing with the "galactic wind": the gas is blown above the galacticplane with the characteristic velocity of about 130km/s. The gas outflow is caused by a combined action of winds from the ...
... The RATAN Radio continuum survey of the Galacticplane between l=342^o and l=17^o ... THE Ratan radio continuum survey of the Galacticplane bet- ween l = 343^o AND l ...
... center of the system and ab out 20 p c toward to the north of the galacticplane ... lines (He-rich, He-weak) show conspicuous concentration towards the galacticplane ...
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... The images were rotated to align the galacticplane parallel to the horizontal axis. ... The radial profile drawn through the galacticplane is shown in the middle panels of ... Here jzj designates the distance to the galacticplane. ...
... and, third, small areas in the Galacticplane where the distribution of interstellar ... of its emission near the Galacticplane, its observed angular characteristics are ...