VOSED A tool for Building Spectral Energy Distributions. Comparison with theoretical models Raúl Gutiérrez [email protected] E. Solano, L. M. Sarro, B.
The herschel view_of_massive_star_formation_in_dense_and_cold_filament_w48
The most luminous_galaxies_discovered_by_wise
New insights from aperiodic variability of young stars
PF-STAR: emotional speech synthesis Istituto di Scienze e Tecnologie della Cognizione, Sezione di Padova – “Fonetica e Dialettologia”, CNR.
References [1] Liseau R., Lorenzetti D., Nisini B. et al. 1992 A&A 265, 577 [2] Massi F., De Luca M., Elia D. et al. 2006 A&A, submitted 399,14 [3] C.A.
From Pre-stellar Cores to Proto-stars: The Initial Conditions of Star Formation PHILIPPE ANDRE DEREK WARD-THOMPSON MARY BARSONY Reported by Fang Xiong,
Extrasolar planet detection: Methods and limits Ge/Ay133.
The monitoring of GRB afterglows and the study of their host galaxies with the SAO RAS 6-m telescope from 1997 V. Sokolov et al. The review of main results.
From Pre-stellar Cores to Proto-stars: The Initial Conditions of Star Formation
Rise and Fall of the X-ray flash 080330: an off-axis jet? C.Guidorzi 1,2,3 on behalf of a large collaboration of the Swift, Liverpool and Faulkes Telescopes,
T Pyx
![References [1] Liseau R., Lorenzetti D., Nisini B. et al. 1992 A&A 265, 577 [2] Massi F., De Luca M., Elia D. et al. 2006 A&A, submitted 399,14 [3] C.A.](https://static.fdocuments.net/doc/330x215/56649cb05503460f94974367/references-1-liseau-r-lorenzetti-d-nisini-b-et-al-1992-aa-265-577.jpg)
