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The turbulent birth of stars in galactic collisions

(PresseBox) (Bruxelles, )
Using very high-resolution numerical simulations, astrophysicists at the CEA and CNRS, led by Florent Renaud , have, for the very first time, achieved a detailed analysis of the effects of turbulence generated when two galaxies collide. These numerical simulations, in which the disordered motions of the gas contained in galaxies are seen at extremely small-scale resolutions, at last explain a phenomenon that astrophysicists have observed but which they have been unable to understand until now: that of "starbursts" of star formation when galaxies collide. A process of compressive turbulence helps to explain such starbursts, and why some galaxies form more vdbru frkz mwithj. Fwydc iteugob xsx zfpcqcjfp mx Opsfieg Peqlyvy ek mjy Txtbu Abmstlapfiwt Yagdwhp, Xgiklxh, Noe 1695.

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The publisher indicated in each case (see company info by clicking on image/title or company info in the right-hand column) is solely responsible for the stories above, the event or job offer shown and for the image and audio material displayed. As a rule, the publisher is also the author of the texts and the attached image, audio and information material. The use of information published here is generally free of charge for personal information and editorial processing. Please clarify any copyright issues with the stated publisher before further use. In case of publication, please send a specimen copy to service@pressebox.de.