Objetivo The aim of this project is to obtain the highest quality observations of the atomic interstellar medium (ISM), through observations of the 21cm line of atomic hydrogen, ever made of a substantial sample of nearby galaxies, covering a wide range of Hubble types, star formation rates, absolute luminosities, evolutionary stages, and metallicities in order to derive the detailed morphology, three-dimensional structure, and mass distribution of galaxies in the nearby Universe.Particular emphasis will be placed o n the interplay between the ISM and Star Formation, the Star Formation threshold as a function of Hubble Type and metallicity, and the physical characteristics of the cool and warm neutral ISM as traced by neutral hydrogen. Ámbito científico natural sciencesphysical sciencesastronomyobservational astronomyoptical astronomynatural sciencesphysical sciencesastronomyobservational astronomyradio astronomynatural sciencesphysical sciencesastronomyastrophysicsdark matternatural sciencesphysical sciencesastronomyplanetary sciencescelestial mechanicsnatural sciencesphysical sciencesastronomyobservational astronomyinfrared astronomy Programa(s) FP6-MOBILITY - Human resources and Mobility in the specific programme for research, technological development and demonstration "Structuring the European Research Area" under the Sixth Framework Programme 2002-2006 Tema(s) MOBILITY-4.2 - Marie Curie International Reintegration Grants (IRG) Convocatoria de propuestas FP6-2002-MOBILITY-12 Consulte otros proyectos de esta convocatoria Régimen de financiación IRG - Marie Curie actions-International re-integration grants Coordinador THE UNIVERSITY OF HERTFORDSHIRE Aportación de la UE Sin datos Dirección College Lane HATFIELD Reino Unido Ver en el mapa Enlaces Sitio web Opens in new window Coste total Sin datos
