Magnetic Fields
Throughout Stellar Evolution
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Program
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List
‹
Monday, August 26, 2013
›
09:00
10:00
11:00
12:00
13:00
14:00
15:00
16:00
17:00
18:00
›9:00 (05min)
Welcome address
Pascal Petit
9:00 - 9:05 (05min)
Welcome address
Pascal Petit
›9:05 (40min)
General Introduction
9:05 - 9:45 (40min)
General Introduction
›
Magnetic Fields in Stars: Origin and Impact
- Norbert Langer, Argelander Institute for Astronomy
09:05-09:45 (40min)
›9:45 (50min)
Session 1 - Magnetized stellar formation
Chair: Gregg Wade
9:45 - 10:35 (50min)
Session 1 - Magnetized stellar formation
Chair: Gregg Wade
›
The role of magnetic fields in star formation
- Ralph Pudritz, Dept. of Physics and Astronomy, McMaster University
09:45-10:15 (30min)
›
Magnetic field dispersion in the neighbourhood of Bok globules
- Claudia Rodrigues, Instituto Nacional de Pesquisas Espaciais
10:15-10:35 (20min)
›10:35 (30min)
Coffee break
10:35 - 11:05 (30min)
Coffee break
›11:05 (1h10)
Session 1 - Magnetized stellar formation
Chair: Gregg Wade
11:05 - 12:15 (1h10)
Session 1 - Magnetized stellar formation
Chair: Gregg Wade
›
The role of magnetic fields in pre-main sequence stars
- Gaitee Hussain, European Southern Observatory
11:05-11:35 (30min)
›
Can we predict the global magnetic topology of a pre-main sequence star from its position in the Hertzsprung-Russell diagram?
- Scott Gregory, University of St. Andrews
11:35-11:55 (20min)
›
Analysis of Star-Disk Interaction in Young Stellar Systems
- Nathalia Fonseca, Universidade Federal de Minas Gerais
11:55-12:15 (20min)
›12:15 (2h)
Lunch
12:15 - 14:15 (2h)
Lunch
›14:15 (1h40)
Session 1 - Magnetized stellar formation
Chair: Corinne Charbonnel
14:15 - 15:55 (1h40)
Session 1 - Magnetized stellar formation
Chair: Corinne Charbonnel
›
Magnetospheric accretions and outflows in young stellar objects
- Ryuichi Kurosawa, Max-Planck-Institute for Radio Astronomy
14:15-14:45 (30min)
›
3D YSO accretion shock simulations: a study of the magnetic, chromospheric and stochastic flow effects and their observational relevance
- Titos Matsakos, Laboratoire AIM, CEA/DSM - CNRS - Université Paris Diderot, IRFU/Service d'Astrophysique, CEA Saclay, CEA, IRAMIS, Service Photons, Atomes et Molécules
14:45-15:05 (20min)
›
Magnetic higher-mass stars in the early stages of their evolution
- Jason Grunhut, European Southern Observatory
15:05-15:35 (30min)
›
What do weak magnetic fields mean for magnetospheric accretion in Herbig AeBe star+disk systems?
- Alicia Aarnio, University of Michigan
15:35-15:55 (20min)
›15:55 (30min)
Coffee break
15:55 - 16:25 (30min)
Coffee break
›16:25 (1h30)
Session 1 - Magnetized stellar formation
Chair: Corinne Charbonnel
16:25 - 17:55 (1h30)
Session 1 - Magnetized stellar formation
Chair: Corinne Charbonnel
›
Chemical peculiarities in magnetic and non-magnetic pre-main sequence A and B stars
- Colin Folsom, Institut de recherche en astrophysique et planétologie
16:25-16:45 (20min)
›
Angular momentum evolution of young stars
- Stuart Littlefair, University of Sheffield
16:45-17:15 (30min)
›
Activity and Rotation in the young cluster h Per
- Costanza Argiroffi, Dip. di Fisica e Chimica, Universita' di Palermo
17:15-17:35 (20min)
›
X-ray emission regimes and rotation sequences in the M34 open cluster
- Philippe Gondoin, European Space and Technology Centre
17:35-17:55 (20min)
›17:55 (20min)
Session 2 - Magnetic activity in the Sun and main-sequence stars with convective outer layers
Chair: Corinne Charbonnel
17:55 - 18:15 (20min)
Session 2 - Magnetic activity in the Sun and main-sequence stars with convective outer layers
Chair: Corinne Charbonnel
›
Do Magnetic Fields Actually Inflate Low-Mass Stars?
- Gregory Feiden, Department of Physics and Astronomy, Dartmouth College, Department of Physics and Astronomy, Uppsala University
17:55-18:15 (20min)
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