Symposium S11  11-12 July 2023

Stellar interactions: contact binary stars and common-envelope evolution

Aims and scope

Interacting stars and their evolutionary products are important for nearly every branch of astronomy. In this symposium, we focus on two particularly crucial and still incompletely understood kinds of stellar interactions where the stars of a binary system share an envelope:

1) The contact binary phase.
2) The common envelope phase.

These types of stellar interactions impact the formation and evolution of diverse exotic phenomena such as compact objects, X-ray binaries, stellar mergers, gravitational-wave sources, luminous red novae, supernovae, gamma-ray bursts and the dynamics of triples and higher-order multiples, among others.

The common envelope phase occurs in various stellar binaries that undergo unstable mass transfer, where on short timescales the stellar cores spiral in and form a close binary or merge, and some or all of the envelope is ejected. On the other hand, if a short-period binary on the main sequence undergoes stable mass transfer and both stars simultaneously overflow their Roche lobes, a contact system may form. Such contact binaries have been observed in the Milky Way and Magellanic Clouds.

Thanks to recent modeling and observational advances, the fields of contact binary stars and common envelope evolution are rapidly developing. The main goal of this symposium is to gather the observational and modeling communities working on common envelopes and contact binaries on a common platform to examine our current knowledge and create fruitful collaborations to advance our understanding of these pivotal phases of stellar dynamics.

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• VFTS 352 Contact Binary Image Credit: ESO/L. Calçada
• Common Envelope Simulation Image Credit: H.Glanz


Programme


How common envelope evolution affects stellar systems
Observations of high-mass contact binaries in the local Universe

The physics of common envelope evolution
Observations of diverse types of low-mass contact binaries

Progenitors, transients, and remnants of the common envelope phase
Modelling of contact binaries across all masses

Invited speakers


Paul Ricker
University of Illinois Urbana-Champaign

Michael Abdul-Masih
European Southern Observatory: Santiago

Nadia Blagorodnova
University of Barcelona

Kosmas Gazeas
University of Athens

Alejandro Vigna Gomez
Max Planck Institute for Astrophysics

Pablo Marchant
KU Leuven

Scientific organisers

Hila Glanz (chair)
Technion - Israel Institute of Technology
Athira Menon (chair)
Institute of Astrophysics of the Canary Islands
Alexey Bobrick (chair)
Technion - Israel Institute of Technology
Silvia Toonen
University of Amsterdam
Tomasz Kaminski
Nicolaus Copernicus Center
Alex de Koter
University of Amsterdam
Friedrich Roepke
Heidelberg Institute for Theoretical Studies
Norbert Langer
University of Bonn
Morgan MacLeod
CfA, Harvard & Smithsonian
Kosmas Gazeas
University of Athens
Laurent Mahy
Royal Observatory of Belgium

Contact

HilaGlanz @ gmail.com amenon @ iac.es a.l.bobrick @ gmail.com

Updated on Tue Mar 07 17:26:27 CET 2023