Hostname: page-component-cd9895bd7-mkpzs Total loading time: 0 Render date: 2024-12-21T12:53:49.306Z Has data issue: false hasContentIssue false

A Wide Angle Search for Hot Jupiters and Pre-Main Sequence Binaries in Young Stellar Associations

Published online by Cambridge University Press:  27 January 2016

Ryan J. Oelkers
Affiliation:
George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Dept. of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA
Lucas M. Macri
Affiliation:
George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Dept. of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA
Jennifer L. Marshall
Affiliation:
George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Dept. of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA
Darren L. DePoy
Affiliation:
George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Dept. of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA
Carlos Colazo
Affiliation:
Observatorio Astronómico, Universidad Nacional de Córdoba
Pablo Guzzo
Affiliation:
Observatorio Astronómico, Universidad Nacional de Córdoba
Diego G. Lambas
Affiliation:
Observatorio Astronómico, Universidad Nacional de Córdoba Instituto de Astronomía Teórica y Experimental, IATE-CONICET email: ryan.oelkers@physics.tamu.edu
Ceci Quiñones
Affiliation:
Observatorio Astronómico, Universidad Nacional de Córdoba
Katelyn Stringer
Affiliation:
George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Dept. of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA
Luis Tapia
Affiliation:
Observatorio Astronómico, Universidad Nacional de Córdoba
Colin Wisdom
Affiliation:
George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Dept. of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The past two decades have seen a significant advancement in the detection, classification and understanding of exoplanets and binary star systems. The vast majority of these systems consist of stars on the main sequence or on the giant branch, leading to a dearth of knowledge of properties at early times (<50 Myr). Only one transiting planet candidate and a dozen eclipsing binaries are known among pre-main sequence objects, yet these are the systems that can provide the best constraints on stellar and planetary formation models. We have recently completed a photometric survey of 3 young (<50 Myr), nearby (D<150 pc) moving groups with a small-aperture instrument, nicknamed “AggieCam”. We detected 7 candidate Hot Jupiters and over 200 likely pre-main sequence binaries, which are now being followed up photometrically and spectroscopically.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2016 

References

Kovács, G., Zucker, S., & Mazeh, T. 2002, A&A, 391, 369Google Scholar
Lomb, N. R. 1976, Ap&SS, 39, 447Google Scholar
McCarthy, J. K., Sandiford, B. A., Boyd, D., & Booth, J. 1993, PASP, 105, 881Google Scholar
Oelkers, R. J., Macri, L. M., Wang, L., Ashley, M. C. B., Cui, X., Feng, L.-L., Gong, X., Lawrence, J. S., Qiang, L., Luong-Van, D., Pennypacker, C. R., Yang, H., Yuan, X., York, D. G., Zhou, X., & Zhu, Z. 2015, AJ, 149, 50Google Scholar
Pettersson, B., 2008, in Handbook of Star Forming Regions, Volume II, 43, ed. Reipurth, B. (San Francisco: Astronomical Society of the Pacific)Google Scholar
Scargle, J. D. 1982, ApJ, 263, 835Google Scholar