... Possible mechanisms of exchange are: galactic wind driven by multiple explosions of SNae ram pressure of intergalacticgas tidal action from nearby galaxies evaporation of gas by hot IGM blow out of dust by star radiation pressure accretion from IGM ...
... Is is believed that the formation of PRGs is in most cases caused by galaxy mergers with the corresponding direction of angular momentum, the accretion by the host galaxy of the companion's matter, or gas filaments from the intergalactic medium. ...
... It is believed that PRGs in most cases are formed by either the merger of galaxies with the specific spin orientation or the accretion by the host galaxy of the companion matter or gas clouds from the intergalactic medium. ...
... only 5% of their observed luminosity. b) S and Im,BCD galaxies possess the supply of gas sufficient to maintain their observed SFRs during only next (1/4 - 1/3)T0 years, while dIr and dSph populations have the mean gas depletion time about 3 T0 ...
... V.V., Karachentsev I.D. Detection of an Intergalactic Meteor Particle with the 6-m ... A., Moiseev A.V., Egorov O.V. Gas Emission Spectrum in a Star-Forming Region in the ...
... of stars and the star formation rate depends on the supply of gas to the arms ... with explanation of elemental pattern in the intergalactic medium, Ly-alpha forest ... negative feedback preventing formation of stellar population in primeval gas ...