Tamura_SWG_StarForma..
DW-MRI and MRS to Differentiate Radiation Necrosis and Recurrent ...
Mrk334: is a connection between nucleus activity and merging of a companion? Smirnova A.A., Moiseev A.V., Afanasiev V.L. Special Astrophysical Observatory.
Samansa Maneshi, Jalani Kanem, Chao Zhuang, Matthew Partlow Aephraim Steinberg Department of Physics, Center for Quantum Information and Quantum Control,
CDM cusps in LSB galaxies by means of stellar kinematics A.Pizzella, E.M.Corsini, F. Bertola Università di Padova And J. Magorrian, M. Sarzi University.
The Emission Line Universe
1 High-z galaxy masses from spectroastrometry Alessio Gnerucci Department of Physics and Astronomy University of Florence 13/12/2009- Obergurgl Collaborators:
Handling 3D Data in the Virtual Observatory Igor Chilingarian (CRAL Observatoire de Lyon, France/SAI MSU, Russia) Francois Bonnarel (CDS Observatoire de.
Synergies between ALMA and VLT(I)
Central Engine of AGN Xi’ian 15-21 October 2006
OWL Instrument Concept Studies Within the OWL Conceptual Design to be completed by ESO in 3Q 2005, ESO collaborates with external institutes in the study.
The central 80x200 pc of M83:how many BH and how massive are they?
