Fundamental Stellar Properties from Optical Interferometry

G. T. van Belle; J. Aufdenberg; T. Boyajian; [No Value] Harper G.; C. Hummel; E. Pedretti; E. Baines; R. White; V. Ravi; S. Ridgway

Fundamental Stellar Properties from Optical Interferometry

G. T. van Belle
, J. Aufdenberg
, T. Boyajian
, [No Value] Harper G.
, C. Hummel
, E. Pedretti
, E. Baines
, R. White
, V. Ravi
, S. Ridgway

The Scottish Association for Marine Science, Scottish Marine Institute

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Resumen

High-resolution observations by visible and near-infrared interferometers of both single stars and binaries have made significant contributions to the foundations that underpin many aspects of our knowledge of stellar structure and evolution for cool stars. The CS16 splinter on this topic reviewed contributions of optical interferometry to date, examined highlights of current research, and identified areas for contributions with new observational constraints in the near future.

Idioma original	English
Título de la publicación alojada	16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun
Subtítulo de la publicación alojada	proceedings of a conference held August 28- September 2, 2010 at the University of Washington, Seattle, Washington
Lugar de publicación	Cambridge
Editorial	ASP
Páginas	517
Volumen	448
Estado	Published - 1 dic 2011

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http://adsabs.harvard.edu/abs/2011ASPC..448..517V

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van Belle, G. T., Aufdenberg, J., Boyajian, T., Harper G., N. V., Hummel, C., Pedretti, E., Baines, E., White, R., Ravi, V., & Ridgway, S. (2011). Fundamental Stellar Properties from Optical Interferometry. En 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun: proceedings of a conference held August 28- September 2, 2010 at the University of Washington, Seattle, Washington (Vol. 448, pp. 517). ASP. http://adsabs.harvard.edu/abs/2011ASPC..448..517V

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title = "Fundamental Stellar Properties from Optical Interferometry",

abstract = "High-resolution observations by visible and near-infrared interferometers of both single stars and binaries have made significant contributions to the foundations that underpin many aspects of our knowledge of stellar structure and evolution for cool stars. The CS16 splinter on this topic reviewed contributions of optical interferometry to date, examined highlights of current research, and identified areas for contributions with new observational constraints in the near future.",

author = "\{van Belle\}, \{G. T.\} and J. Aufdenberg and T. Boyajian and \{Harper G.\}, \{[No Value]\} and C. Hummel and E. Pedretti and E. Baines and R. White and V. Ravi and S. Ridgway",

year = "2011",

month = dec,

day = "1",

language = "English",

volume = "448",

pages = "517",

booktitle = "16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun",

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van Belle, GT, Aufdenberg, J, Boyajian, T, Harper G., NV, Hummel, C, Pedretti, E, Baines, E, White, R, Ravi, V & Ridgway, S 2011, Fundamental Stellar Properties from Optical Interferometry. En 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun: proceedings of a conference held August 28- September 2, 2010 at the University of Washington, Seattle, Washington. vol. 448, ASP, Cambridge, pp. 517. <http://adsabs.harvard.edu/abs/2011ASPC..448..517V>

TY - GEN

T1 - Fundamental Stellar Properties from Optical Interferometry

AU - van Belle, G. T.

AU - Aufdenberg, J.

AU - Boyajian, T.

AU - Harper G., [No Value]

AU - Hummel, C.

AU - Pedretti, E.

AU - Baines, E.

AU - White, R.

AU - Ravi, V.

AU - Ridgway, S.

PY - 2011/12/1

Y1 - 2011/12/1

N2 - High-resolution observations by visible and near-infrared interferometers of both single stars and binaries have made significant contributions to the foundations that underpin many aspects of our knowledge of stellar structure and evolution for cool stars. The CS16 splinter on this topic reviewed contributions of optical interferometry to date, examined highlights of current research, and identified areas for contributions with new observational constraints in the near future.

AB - High-resolution observations by visible and near-infrared interferometers of both single stars and binaries have made significant contributions to the foundations that underpin many aspects of our knowledge of stellar structure and evolution for cool stars. The CS16 splinter on this topic reviewed contributions of optical interferometry to date, examined highlights of current research, and identified areas for contributions with new observational constraints in the near future.

M3 - Conference contribution

VL - 448

SP - 517

BT - 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun

PB - ASP

CY - Cambridge

ER -

Fundamental Stellar Properties from Optical Interferometry

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