Imaging rapid rotators with the PAVO beam combiner at CHARA

Vicente Maestro; Yitping Kok; Daniel Huber; Michael J. Ireland; Peter G. Tuthill; Tim White; Gail Schaefer; Theo A. Ten Brummelaar; Harold A. McAlister; Nils Turnere; Christopher D. Farrington; P. J. Goldfinger

doi:10.1117/12.926881

Imaging rapid rotators with the PAVO beam combiner at CHARA

Vicente Maestro^*, Yitping Kok, Daniel Huber, Michael J. Ireland, Peter G. Tuthill, Tim White, Gail Schaefer, Theo A. Ten Brummelaar, Harold A. McAlister, Nils Turnere, Christopher D. Farrington, P. J. Goldfinger

^*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution › peer-review

5 Citations (Scopus)

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Abstract

Rotation plays a crucial role in the shaping and evolution of a star. Widely incorporated into early and late-stage stellar models, rotational effects remain poorly understood in main-sequence stars, mainly due to the absence of observations challenging contemporary models. The Precision Astronomical Visible Observations (PAVO) instrument, located at the Center for High Angular Resolution Astronomy (CHARA) array, provides the highest angular resolution yet achieved ( 0.3 mas) for stars V=8 magnitude and brighter. We describe instrumental techniques and advances implemented in PAVO@CHARA to observe heavily resolved targets and yield well calibrated closure phases which are key milestones on the pathway to delivery of the first-ever image in the visible of fast-rotating main-sequence star.

Original language	English
Title of host publication	Optical and Infrared Interferometry III
Editors	Françoise Delplancke, Jayadev K. Rajagopal, Fabien Malbet
Place of Publication	Bellingham, Washington
Publisher	SPIE
Pages	1-15
Number of pages	15
Volume	8445
ISBN (Print)	9780819491466
DOIs	https://doi.org/10.1117/12.926881
Publication status	Published - 2012
Event	Optical and Infrared Interferometry III - Amsterdam, Netherlands Duration: 1 Jul 2012 → 6 Jul 2012

Other

Other	Optical and Infrared Interferometry III
Country/Territory	Netherlands
City	Amsterdam
Period	1/07/12 → 6/07/12

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Maestro, V., Kok, Y., Huber, D., Ireland, M. J., Tuthill, P. G., White, T., Schaefer, G., Ten Brummelaar, T. A., McAlister, H. A., Turnere, N., Farrington, C. D., & Goldfinger, P. J. (2012). Imaging rapid rotators with the PAVO beam combiner at CHARA. In F. Delplancke, J. K. Rajagopal, & F. Malbet (Eds.), Optical and Infrared Interferometry III (Vol. 8445, pp. 1-15). Article 84450G SPIE. https://doi.org/10.1117/12.926881

@inproceedings{cc70523e69cd4b1cbb377f224927735d,

title = "Imaging rapid rotators with the PAVO beam combiner at CHARA",

abstract = "Rotation plays a crucial role in the shaping and evolution of a star. Widely incorporated into early and late-stage stellar models, rotational effects remain poorly understood in main-sequence stars, mainly due to the absence of observations challenging contemporary models. The Precision Astronomical Visible Observations (PAVO) instrument, located at the Center for High Angular Resolution Astronomy (CHARA) array, provides the highest angular resolution yet achieved ( 0.3 mas) for stars V=8 magnitude and brighter. We describe instrumental techniques and advances implemented in PAVO@CHARA to observe heavily resolved targets and yield well calibrated closure phases which are key milestones on the pathway to delivery of the first-ever image in the visible of fast-rotating main-sequence star.",

author = "Vicente Maestro and Yitping Kok and Daniel Huber and Ireland, {Michael J.} and Tuthill, {Peter G.} and Tim White and Gail Schaefer and {Ten Brummelaar}, {Theo A.} and McAlister, {Harold A.} and Nils Turnere and Farrington, {Christopher D.} and Goldfinger, {P. J.}",

year = "2012",

doi = "10.1117/12.926881",

language = "English",

isbn = "9780819491466",

volume = "8445",

pages = "1--15",

editor = "Fran{\c c}oise Delplancke and Rajagopal, {Jayadev K.} and Fabien Malbet",

booktitle = "Optical and Infrared Interferometry III",

publisher = "SPIE",

address = "United States",

note = "Optical and Infrared Interferometry III ; Conference date: 01-07-2012 Through 06-07-2012",

}

Maestro, V, Kok, Y, Huber, D, Ireland, MJ, Tuthill, PG, White, T, Schaefer, G, Ten Brummelaar, TA, McAlister, HA, Turnere, N, Farrington, CD & Goldfinger, PJ 2012, Imaging rapid rotators with the PAVO beam combiner at CHARA. in F Delplancke, JK Rajagopal & F Malbet (eds), Optical and Infrared Interferometry III. vol. 8445, 84450G, SPIE, Bellingham, Washington, pp. 1-15, Optical and Infrared Interferometry III, Amsterdam, Netherlands, 1/07/12. https://doi.org/10.1117/12.926881

Imaging rapid rotators with the PAVO beam combiner at CHARA. / Maestro, Vicente; Kok, Yitping; Huber, Daniel et al.
Optical and Infrared Interferometry III. ed. / Françoise Delplancke; Jayadev K. Rajagopal; Fabien Malbet. Vol. 8445 Bellingham, Washington: SPIE, 2012. p. 1-15 84450G.

Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution › peer-review

TY - GEN

T1 - Imaging rapid rotators with the PAVO beam combiner at CHARA

AU - Maestro, Vicente

AU - Kok, Yitping

AU - Huber, Daniel

AU - Ireland, Michael J.

AU - Tuthill, Peter G.

AU - White, Tim

AU - Schaefer, Gail

AU - Ten Brummelaar, Theo A.

AU - McAlister, Harold A.

AU - Turnere, Nils

AU - Farrington, Christopher D.

AU - Goldfinger, P. J.

PY - 2012

Y1 - 2012

N2 - Rotation plays a crucial role in the shaping and evolution of a star. Widely incorporated into early and late-stage stellar models, rotational effects remain poorly understood in main-sequence stars, mainly due to the absence of observations challenging contemporary models. The Precision Astronomical Visible Observations (PAVO) instrument, located at the Center for High Angular Resolution Astronomy (CHARA) array, provides the highest angular resolution yet achieved ( 0.3 mas) for stars V=8 magnitude and brighter. We describe instrumental techniques and advances implemented in PAVO@CHARA to observe heavily resolved targets and yield well calibrated closure phases which are key milestones on the pathway to delivery of the first-ever image in the visible of fast-rotating main-sequence star.

AB - Rotation plays a crucial role in the shaping and evolution of a star. Widely incorporated into early and late-stage stellar models, rotational effects remain poorly understood in main-sequence stars, mainly due to the absence of observations challenging contemporary models. The Precision Astronomical Visible Observations (PAVO) instrument, located at the Center for High Angular Resolution Astronomy (CHARA) array, provides the highest angular resolution yet achieved ( 0.3 mas) for stars V=8 magnitude and brighter. We describe instrumental techniques and advances implemented in PAVO@CHARA to observe heavily resolved targets and yield well calibrated closure phases which are key milestones on the pathway to delivery of the first-ever image in the visible of fast-rotating main-sequence star.

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U2 - 10.1117/12.926881

DO - 10.1117/12.926881

M3 - Conference proceeding contribution

AN - SCOPUS:84873025815

SN - 9780819491466

VL - 8445

SP - 1

EP - 15

BT - Optical and Infrared Interferometry III

A2 - Delplancke, Françoise

A2 - Rajagopal, Jayadev K.

A2 - Malbet, Fabien

PB - SPIE

CY - Bellingham, Washington

T2 - Optical and Infrared Interferometry III

Y2 - 1 July 2012 through 6 July 2012

ER -

Imaging rapid rotators with the PAVO beam combiner at CHARA

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