... indicates that we are dealing with the "galactic wind": the gas is blown above the galactic plane with the characteristic velocity of about 130km/s. The gas outflow is caused by a combined action of winds from the supernovae and young massive stars ...
... An increase in star brightness is followed by a decrease in asphericity and wind velocity to the point where stationary and even accreting fraction of the wind appears in extremely bright objects together with a flowing out fraction. ...
... Temperature: . 8.2 C . Wind Chill: . 8.2 C . Heat Index: . 8.2 C . ... Barometer: . 784.6 mb - . Wind: . S at 0.0 km/h . High Wind: . 34 km/h at 16:45 . ... Wind: . S at 0.0 km/h . High Wind: . 34 km/h at 16:45 . Recent Avg Wind: . 0 km/h . ...
... Fig.2. The first computer model of the supercritical-disk wind. ... The wind is ejected as a hollow cone; it has a funnel (the funnel opening angle in ... right, and sees everything up to the wind photosphere (the red color in the figure ...
... of 1 cm indications have been found of existence of relativistic electrons in the magnetosphere of Jupiter with energy of about 100 MeV, which demands revision of mechanisms of acceleration of cosmic rays of the solar wind with energy of a few MeV ...
... GCN GRB Report No 4809) of type Ic we detected a spectral detail which is interpreted as the H_alpha line (P-Cyg absorption) component that can be connected to an envelope which usually arises around a massive progenitor star due to stellar wind. ...
... wind driven by multiple explosions of SNae ram pressure of intergalactic gas tidal action from nearby galaxies evaporation of gas by hot IGM blow out of dust by star radiation pressure accretion from IGM escape of stars with velo cities large enough ...
... wind (Porter, 1997) corresponding to the field B = 100 G (top), and the expected ... magnetized winds and negligible for a spherically symmetric geometry of the wind ...
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