26 Maggio, 2010 AGN9 - FERRARA Poster(s) Radio quieti … + SKA Photos : Marcella Brusa.
A 3d extinction_map_of_the_northern_galactic_plane_based_on_iphas_photometry
ASTR112 The Galaxy Lecture 7 Prof. John Hearnshaw 11. The galactic nucleus and central bulge 11.1 Infrared observations (cont.) 11.2 Radio observations.
Rich cluster [M ~ 10 15 M sun ] Large groups (Small clusters) [M ~ 10 13 - 10 14 M sun ] Environmental effects on neutral and molecular hydrogen of galaxies.
Ringberg 17 April 2004Modeling Structure, Chemistry, Appearance of Protoplanetary Disks.1 Modeling the structure, chemistry and appearance of protoplanetary.
Mapping the circumnuclear dust in nearby AGN with MIDI Konrad R.W. Tristram, Klaus Meisenheimer Max-Planck-Institut für Astronomie Heidelberg, Germany.
The WFIRST Microlensing Exoplanet Survey: Figure of Merit David Bennett University of Notre Dame WFIRST.
Mercury Disk Observations by Japanese team 1. Observation of Mercury transit on the solar disk
Poster(s)
A Summary of Results from Nulling Interferometry W. Liu, P. Hinz, W. Hoffmann, and the MMT Adaptive Optics Group Steward Observatory, University of Arizona.
Modeling the structure, chemistry and appearance of protoplanetary disks
Mapping the circumnuclear dust in nearby AGN with MIDI
![Rich cluster [M ~ 10 15 M sun ] Large groups (Small clusters) [M ~ 10 13 - 10 14 M sun ] Environmental effects on neutral and molecular hydrogen of galaxies.](https://static.fdocuments.us/doc/330x215/56649d315503460f94a0a1da/rich-cluster-m-10-15-m-sun-large-groups-small-clusters-m-10-13-.jpg)
