Seeding the local disk galaxy population

Details Seeding the local disk galaxy population Seeding the local disk galaxy population

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40...84r&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Dark Matter, Galaxies: Luminosity Function, Mass Function, Galaxies: Spiral

Scientific paper

By means of the abundance matching technique we have inferred the local stellar & baryonic-halo mass (M_s & M_b-M_h) relations for central blue and red galaxies. Models of disk galaxies loaded inside Λ Cold Dark Matter (ΛCDM) halos are used to probe the obtained blue M_b-M_h relation in the light of observed scaling relations.

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