G1 – Commission G1 Binary and Multiple Star Systems

Description

Binary and multiple stellar systems are an essential part of stellar physics, since single stars like the Sun are shown to be in the minority. Binary stars provide the most tractable, calibration-free path to fundamental stellar parameters (masses, radii, luminosities and temperatures). They also have vital interactions with planetary science, stellar structure and evolution (as calibrators), high energy astrophysics, galactic chemical evolution by way of supernovae, and cosmology. Binary stars also serve as standard distance calibrators, where the precision in the determined distance does not depend on the distance itself. The intent is to include all relevant kinds of observations of individual systems and populations, statistical studies, both analytical and numerical calculations, and database maintenance.

The main science topics central to the Commission are:

• the full range of observational tools that reveal binary and multiple systems (astrometry, photometry, spectroscopy, polarimetry, structure of cluster HR diagrams, products of space missions including Kepler, Gaia and LSST), and the interface of these with concerns of other Divisions and Commissions;
• kinematics, and ultimately dynamics, of binary and multiple systems;
• improved codes for binary and multiple systems, stellar atmospheres, structure and evolution, yielding surface compositions, tracks in the HR diagram, temporal changes in system masses and separations, etc;
• improvements of existing binary and multiple star system databases, regular production of publications (online and perhaps in print on paper), sharing databases, new codes, exciting discoveries, and opportunities for interaction with other parts of the astronomical community; and
• accurate knowledge of the history of the subject and its continuing impact on astronomy in general.

External page:  http://www.astro.gsu.edu/wds/bsl/

Commission Web Page

Commission Members (304)

Under Division

Division G Stars and Stellar Physics

President

Virginia Trimble

University of California Irvine
Physics-Astronomy Department
4575 Physics
Irvine CA 92697-4575
California (CA)
United States

Phone: +1 949 824 6948
Email 1: vtrimbleuciedu
Email 2: vtrimbleastroumdedu
Organization website: http://www.physics.uci.edu/

NCA adherence: United States

Last updated:
November 15, 2018

Vice-President

Christopher Adam Tout

University of Cambridge
Institute of Astronomy
The Observatories
Madingley Road
Cambridge CB3 0HA
United Kingdom

Phone: +44 1223 337502
Email: catastcamacuk
Personal website: http://www.ast.cam.ac.uk/~cat/
Organization website: http://www.ast.cam.ac.uk/

NCA adherence: United Kingdom

Last updated:
August 7, 2019

Secretary

John Southworth

Keele University
Astrophysics Group
Newcastle-under-Lyme ST5 5BG
United Kingdom

Email 1: astrojskeeleacuk
Email 2: jktaylorkeeleacuk
Personal website: http://www.astro.keele.ac.uk/~jkt/
Organization website: http://www.astro.keele.ac.uk/

NCA adherence: United Kingdom

Last updated:
November 15, 2018

Advisor

Andrej Prša

Villanova University
Dept. of Astrophysics and Planetary Science
800 E Lancaster Ave
Villanova 19085
Pennsylvania (PA)
United States

Phone: +1 610-519-4822
Fax: +1 610-519-6132
Email 1: aprsavillanovaedu
Email 2: aprsa09gmailcom
Organization website: http://www.villanova.edu

NCA adherence: United States

Last updated:
November 9, 2018

Organizing Committee