Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994mnras.270...75p&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Vol. 270, 75.
Astronomy and Astrophysics
Astronomy
28
Scientific paper
Large-scale propagating star formation in galaxies is studied as a self-regulatin process. The model connects the energy injection by star formation with the resultin interstellar structures in a differentially rotating disc. The star formation cycl includes the formation of new stars in groups, multisupernova remnants agglomerafin the gas into supershells, formation of clouds and repeated birth of stars. We investigat the evolution of a galaxy dominated by this cycle and conclude that the predicted radia distributions of H i and H2, the numbers of multisupernova remnants and massiv( cloud complexes, the surface filling factors of shells, the star formation rate (SFR) and the location of the molecular rings are in agreement with the properties of th( observed galaxies. Key words: stars: formation - supernova remnants - galaxies: ISM - galaxies: stella content - galaxies: structure.
Franco Jose
Palous Jan
Tenorio-Tagle Guillermo
No associations
LandOfFree
Star formation in differentially rotating galactic disks: The physics of self-propagation. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Star formation in differentially rotating galactic disks: The physics of self-propagation., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Star formation in differentially rotating galactic disks: The physics of self-propagation. will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1791642