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

SAMS UHI

Publikation: Conference contribution

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.

Originalsprache	English
Titel	16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun
Untertitel	proceedings of a conference held August 28- September 2, 2010 at the University of Washington, Seattle, Washington
Erscheinungsort	Cambridge
Herausgeber (Verlag)	ASP
Seiten	517
Band	448
Publikationsstatus	Published - 1 Dez. 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. in 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 (Band 448, S. 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",

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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. in 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. Bd. 448, ASP, Cambridge, S. 517. <http://adsabs.harvard.edu/abs/2011ASPC..448..517V>

Fundamental Stellar Properties from Optical Interferometry. / van Belle, G. T.; Aufdenberg, J.; Boyajian, T. et al.
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. Band 448 Cambridge: ASP, 2011. S. 517.

Publikation: Conference contribution

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

Abstract

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