Dust coagulation in molecular clouds (Ormel+, 2009)

Details Dust coagulation in molecular clouds (Ormel+, 2009) Dust coagulation in molecular clouds (Ormel+, 2009)

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..35020845o&link_type=abstract

VizieR On-line Data Catalog: J/A+A/502/845. Originally published in: 2009A&A...502..845O

Computer Science

Molecular Clouds, Interstellar Medium, Models

Scientific paper

Quantities (Q) provided in the tables are (see Table 1 of the paper): Q=fmiss fraction of missing collisions Q=Nfk number of fragments in the large component Q=Sf standard deviation in Nf Q=fpwl fraction of mass in the power-law component Q=q slope in the power-law component Q=Cphi change in the filling factor of the large particle component These output quantities are sampled as function of 1. Recipe type: 'Global' or 'Local' 2. Normalized impact parameter 3. Dimensionless energy parameter eps, which is the collision energy divided by a critical energy threshold 4. The initial filling factor of the aggregate (phi) OR, in case of Q=fmiss, the ratio of the outer over the geometrical radius (Ra).
(2 data files).

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