Volume 334, Issue 1-2 pp. 93-96
Original Paper

The kinematics of very low mass dwarfs: Splinter session summary

A.J. Burgasser

Corresponding Author

A.J. Burgasser

Department of Physics, UC San Diego, MC 0424, 9500 Gilman Drive, La Jolla, CA 92093, USA

Department of Physics, UC San Diego, MC 0424, 9500 Gilman Drive, La Jolla, CA 92093, USASearch for more papers by this author
J.K. Faherty

J.K. Faherty

Universidad de Chile, Cerro Calan Camino El Observatorio #1515, Las Condes Santiago, Chile

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S. Schmidt

S. Schmidt

Department of Astronomy, University of Washington, P.O. Box 351580, Seattle, WA 98195, USA

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A.A. West

A.A. West

Department of Astronomy, Boston University, 725 Commonwealth Ave Boston, MA 02215, USA

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M.R. Zapatero Osorio

M.R. Zapatero Osorio

Centro de Astrobiología (CSIC-INTA), Ctra. Ajalvir km 4, E-28850 Torrejón de Ardoz, Madrid, Spain

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J.S. Pineda

J.S. Pineda

California Institute of Technology, Department of Astronomy, 1200 E. California Ave, Pasadena CA, 91125, USA

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B. Burningham

B. Burningham

Centre for Astrophys. Research, Science and Technology Res. Inst., Univ. of Hertfordshire, Hatfield AL10 9AB, UK

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C. Nicholls

C. Nicholls

Department of Physics, UC San Diego, MC 0424, 9500 Gilman Drive, La Jolla, CA 92093, USA

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R. Sanderson

R. Sanderson

Kapteyn Astronomical Institute, P.O. Box 800, 9700 AV Groningen, The Netherlands

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E. Shkolnik

E. Shkolnik

Lowell Observatory, 1400 W. Mars Hill Road, Flagstaff, AZ, 86001, USA

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D. Rodriguez

D. Rodriguez

Universidad de Chile, Cerro Calan Camino El Observatorio #1515, Las Condes Santiago, Chile

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A. Riedel

A. Riedel

Georgia State University, Suite 400, 29 Peachtree Center Ave, Atlanta, GA 30302, USA

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V. Joergens

V. Joergens

Zentrum für Astronomie Heidelberg, Institut für Theoretische Astrophysik, Albert-Ueberle-Str. 2, D-69120 Heidelberg, Germany; Max-Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany

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First published: 06 February 2013

Abstract

Kinematic investigations are being increasingly deployed in studies of the lowest mass stars and brown dwarfs to investigate their origins, characterize their atmospheres, and examine the evolution of their physical parameters. This article summarizes the contributions made at the “Kinematics of Very Low Mass Dwarfs” splinter session. Results discussed include analysis of kinematic distributions of M, L, and T dwarfs; theoretical tools for interpreting these distributions; identifications of very low mass halo dwarfs and wide companions to nearby stars; radial velocity variability among young and very cool brown dwarfs; and the search and identification of M dwarfs in young moving groups. A summary of discussion points at the conclusion of the splinter sesseion is also presented. (© 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)

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