Titlebook: Highlights of Spanish Astrophysics II; Proceedings of the 4 Jaime Zamorano,Javier Gorgas,Jesús Gallego Conference proceedings 2001 Springer

Genetics

VLBI Imaging of the Gravitational Lenses B1422+231 and MG J0414+0534 (VLBI) observations at 8.4 GHz on 23rd November 1997. We present also a lens model for MG J0414+0534, which reproduces the core positions and flux densities of the VLBI images, combining a singular isothermal ellipsoid with external shear, and a singular isothermal sphere to represent, respectively

使成波狀

Daily Monitoring of the Gravitational Lens QSO 2237+0305 at the Nordic Optical Telescope the Nordic Optical Telescope. We report on some technical aspects of the observations and the quality of the data. We have developed a photometric model for obtaining the light-curves of the four QSO components.

BINGE

個(gè)人長(zhǎng)篇演說

SEEK

The Origin of S0 Galaxies in Clustersare modeled as a thin exponential slab of cold gas, a stellar disk, bulge, and dark matter halo. The interaction of galaxy with the ICM is studied by means of a 3-dimensional non-symmetric high-resolution hydrodynamic code for gaseous matter, coupled with a N-body code for the collision-less matter.

exceed

The Galaxy Cluster Coreter potential) on the central cluster environment (shape and normalization of the luminosity function and density profile) and vice versa. We find no significant dependence between the luminosity function of the core cluster galaxies and the above BCG properties. Moreover, there is no apparent segre

eczema

The Coma Cluster of Galaxies: Spectral Classification and Star Formation with the Sloan Digital Sky pic system in June 1999: an observation of the Coma cluster of galaxies. Our data samples the Southern part of this cluster, out to the virial radius. We outline here the main characteristics of the SDSS spectroscopic systems and provide spectral classifications for 196 Coma galaxies. We have invest

MERIT

Star-Forming Galaxies from the UCM-CIDA-YALE Surveyn and evolution of galaxies. The value for the SFR in the local universe is very dependent on the shape of the luminosity function and in particular on the a parameter. The UCM-CIDA-YALE survey (UCY) has grown to address this problem, among others. Using the objective-prism technique, we have been a

旁觀者

智力高

ent on the radar screen of the controller has also increased. Usually controllers manage about 15 aircraft on their position and sometime this number reach a maximum of 20. On the radar screen, aircraft are represented by spots (with some previous positions and their speed vector) and the associated