... 2009A&A...493..511V). So the question on quantitative reliability of the theoretical mo dels of galactic wind is still open. ... of gas exchange Tidal action Every galaxy in cluster undergo a collision at least once in a lifetime (Tutukov 2006ARep ...
... The distribution of clouds by concentrations depends on the galactic latitude. ... The distribution of cloud mass suggests that the merger, rather than fragmentation dominates in collisions. ...
... in the region of 180 degree -3 is not a power form, but has a maximum at n H = 20 - 60 cm -3 depending of galactic latitude ... mass range the process of coalescence in cloud-cloud collisions predominates but the clouds with low masses are evaporated ...
... to increase their masses and densities due to inelastic collisions and rapid cooling ... found that mean clouds linear diameters along Galactic plane are 2.5 times greater ...
... Galactic radio emission at all latitudes, including the regions near the Galactic ... of the Galactic background radio emission is constant over a wide range of galactic ...
... Galactic Gas at High Latitudes: the Southern Polar Cap I. V. Gosachinskij*, G. N. Il ... Galactic latitude than it does in the northern region (Fig. 4, the correlation ... a) and southern (b) Galactic polar caps versus Galactic latitude. any of the ...
... in such stars is especially difficult due to their broad and very variable line profiles caused by the windwind collision ... a space velocity of 32 km/s with respect to the Galactic open cluster system, with the velocity component U = -26 directed ...
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