Title

Brown dwarfs and very low-mass stars: variability in the Pleiades

Authors

Authors

M. Morales-Calderon; D. B. Y. Navascues; J. A. Caballero;E. L. Martin

Comments

Authors: contact us about adding a copy of your work at STARS@ucf.edu

Abbreviated Journal Title

Astro. Nachr.

Keywords

stars : low-mass, brown dwarfs; stars : variables : general; ROTATION PERIODS; SPECTROSCOPY; ACCRETION; CLUSTER; OBJECTS; Astronomy & Astrophysics

Abstract

We present the results of the optical photometric observations of the Pleiades (125 Myr) cluster. The aim of this research is to look for variability, both due to rotation of single stars and the presence of eclipsing binaries. We have used differential photometry and two different methods of statistical analysis of the data. We have found variability in the Pleiades cluster with amplitudes of about 50 mmag and uncertainties of 5 mmag until I=17.9, well within the brown dwarf regime.

Journal Title

Astronomische Nachrichten

Volume

326

Issue/Number

10

Publication Date

1-1-2005

Document Type

Article; Proceedings Paper

Language

English

First Page

1065

Last Page

1067

WOS Identifier

WOS:000234434000046

ISSN

0004-6337

Share

COinS