Division GRm 106, Convention Hall
August 5, Friday
Morning e-Poster 09:45-10:30
Morning Oral Session 10:30-12:00
Div. G-1
David Soderblom & Andrej Prša Division G Status Report
Roel Lefever Towards a more realistic description of Wolf-Rayet atmospheres
Suman Bala A New Monte-Carlo Radiative Transfer Simulation of Cyclotron Resonant Scattering Features
Oleksandr Yushchenko Radioactive elements with long and short decay times in stellar atmospheres
Innocenza Busa Magnetic pressure a necessary contribution to pressure in stellar atmospheres modeling.
Afternoon Oral Session 1 13:30-15:00
Div. G-2
Lisa Bugnet PhD Prize Talk: Characterization of solar-type stars and study of their internal magnetic fields along the evolution: Machine learning for asteroseismology and theoretical constraints for internal magnetic fields.
Allan Sacha BRUN On convection and gravity waves in F stars
Junho Park Shear instabilities and turbulence in radiation zones of rotating stars
Christopher Tout A double magnetic dynamo in cataclysmic variables
Break 15:00-15:15
Afternoon Oral Session 2 15:15-16:45
Div. G-3
Merieme Chadid First Detection of Gravity Modes in RR Lyrae Stars
Vardan Elbakyan Accretion bursts in high-mass protostars
Elnaz Bakhshi THE FIRST PHOTOMETRIC STUDY OF AH MIC CONTACT BINARY SYSTEM
Division G Operations
Afternoon e-Poster 16:45-17:30
August 8, Monday
Morning e-Poster 09:45-10:30
Morning Oral Session 10:30-12:00
Div. G-4
Simon Blouin Decoding the white dwarf fossil record
Natalia Lewandowska Disentangling the mysteries of single pulses from the Crab pulsar
Taeho Ryu Fully relativistic global simulation of tidal disruption event
Bonnie Zaire What does control the large-scale magnetic field configuration of cool stars?
Afternoon Oral Session 1 13:30-15:00
Div. G-5
Steven Goldman A Census of Thermally-Pulsing AGB stars in the Andromeda Galaxy and a First Estimate of their Contribution to the Global Dust Budget
Jielai Zhang Kilonova and Fast Transients- An Untriggered Search
Melike AFSAR Unveiling effective temperatures using line depth ratios in the infrared H and K bands
Kelly Hambleton The Transients and Variable Stars Science Collaboration Roadmap Explained