VizieR Online Data Catalog: Angular-momentum plane for disc galaxies (Mancera Pina+, 2021)

The galaxies used on one relation are not necessarily used in the other relations. This is because for each component (stars, gas, and baryons) we only use the galaxies with convergent stellar/gas/baryonic specific angular momentum profiles (see Mancera Pina et al., 2021A&A...647A..76M, Cat. J/A+A/647/A76)., So, for example, a galaxy with a convergent stellar specific angular momentum profile but without convergent gas and baryonic specific angular momenta profiles, would be used when studying the stellar component but not the gas and baryons. Therefore, such galaxy appear in "stars.dat" but not in the other two files.

(3 data files).