Detailansicht
The Mass of Galaxies at Low and High Redshift
Proceedings of the European Southern Observatory and Universitäts-Sternwarte München Workshop Held in Venice, Italy, 24-26 October 2001, ESO Astrophysics Symposia
ISBN/EAN: 9783540002055
Umbreit-Nr.: 1515042
Sprache:
Englisch
Umfang: xxii, 363 S., 5 farbige Illustr.
Format in cm:
Einband:
gebundenes Buch
Erschienen am 23.01.2003
- Zusatztext
- InhaltsangabeFrom the Contents: The Mass of the Milky Way.- Distant Field BHB Stars and the Mass of the Milky Way.- A Pattern Speed in the Galaxy's OH/IR Stars.- Dark Matter in the Local Group: The Dark Haloes of the Milky Way, M31 and the Draco dSph.- First Evidence for an Extended Dark Halo in the Draco Dwarf Spheroidal.- The Inner Halo of the Draco dSph.- Mass/Light Variations with Environment.- On the Black Hole - Bulge Mass Relation in Active and Inactive Galaxies.- The 2MASS Luminosity, Velocity, and Mass Functions of Galaxies.- Estimating the Mass of Local Disk Galaxies from the NIR Luminosity.- Galaxy Masses: Disks and Their Halos.- Dark Matter in the Center of LSB and Dwarf Galaxies from Halpha Observations.- Galaxy Systems in Low Density Environment: The NGC 4756 System.- The Masses of Dwarf Elliptical Galaxies: First Results from an ESO Large Program.- Estimating the Masses of Dwarf Ellipticals: First VLT Results.- Dynamical Masses of Elliptical Galaxies.
- Kurztext
- Measuring the masses of galaxies as a function of redshift is perhaps one of the most challenging open issues in current astronomical research. The evolution of the baryonic and dark matter components of galaxies is not only a critical test of the hierarchical formation paradigm, but ultimately also provides new clues on the complex interplay between star formation, the cooling and heating of gas and galaxy merging processes. This book reviews current techniques to measure the baryonic (stellar) and dark masses of nearby galaxies, and focusses on ongoing attempts to measure theses same quantities in galaxies at higher and higher redshifts. It also gives room to future perspectives, with special emphasis on new survey projects and satellite missions.