Cel 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. Dziedzina nauki natural sciencesphysical sciencesastronomyobservational astronomyoptical astronomynatural sciencesphysical sciencesastronomyobservational astronomyradio astronomynatural sciencesphysical sciencesastronomyastrophysicsdark matternatural sciencesphysical sciencesastronomyplanetary sciencescelestial mechanicsnatural sciencesphysical sciencesastronomyobservational astronomyinfrared astronomy Program(-y) 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 Temat(-y) MOBILITY-4.2 - Marie Curie International Reintegration Grants (IRG) Zaproszenie do składania wniosków FP6-2002-MOBILITY-12 Zobacz inne projekty w ramach tego zaproszenia System finansowania IRG - Marie Curie actions-International re-integration grants Koordynator THE UNIVERSITY OF HERTFORDSHIRE Wkład UE Brak danych Adres College Lane HATFIELD Zjednoczone Królestwo Zobacz na mapie Linki Strona internetowa Opens in new window Koszt całkowity Brak danych
