Mme
catherine dougados
(ipag)
22/05/2018 14:00
Powerful atomic jets and molecular outflows are observed in young protostars at all stages of active accretion, from the young embedded Class 0 and Class 1 phases to the later optically revealed T Tauri or Class 2 phase. The origin of the ejection, its role in angular momentum extraction and impact on protoplanetary disk evolution remain as fundamental open questions in star formation.
...
Brunella Nisini
(INAF Osservatorio di Roma)
22/05/2018 14:30
I will present a survey of forbidden line emission in a sample of 130 T Tauri stars in the Lupus, Chamaeleon and sigma Ori clouds conducted with the X-shooter instrument. The aim of the survey is to study the occurrence of high velocity jets and slow winds on a statistical bases, and investigate on the connection between the different mass loss phenomena and the source accretion properties.
Dr
Dirk Froebrich
(University of Kent)
22/05/2018 15:00
The talk will present the main results from the UK Wide-field Infrared survey for H2 (UWISH2).
Mme
Fatima Lopez-Martinez
(Instituto de Astrofísica e Ciências do Espaço)
22/05/2018 15:30
Winds and jets are key factors in the evolution of accretion disks in pre-main sequence stars, and deriving their physical properties is one of the most important steps for a full understanding of the connection among outflow, jet and accretion processes. In this work we determine the physical properties of the high velocity component (HVC) and the low velocity component (LVC) emitting region...
Jochen Eislöffel
(Thüringer Landessternwarte)
23/05/2018 10:45
We will present new observations from accretion bursts from young stars.
Dr
Aris Tritsis
(Research School of Astronomy and Astrophysics)
23/05/2018 11:45
Molecular clouds are the birthplaces of stars. Their structure and evolution hold the key to understanding the initial conditions of star and planet formation, and the physics that sets the distribution of masses and multiplicities of newborn stars. However, their complexity, their typically turbulent, filamentary, disordered appearance, and ubiquitous projection effects hinder all efforts to...
