Rotational Modulation of M/L Dwarfs Due to Magnetic Spots
Abstract
We find periodic I-band variability in two ultracool dwarfs, TVLM 513-46546 and 2MASS J00361617+1821104, on either side of the M/L dwarf boundary. Both of these targets are short-period radio transients, with the detected I-band periods matching those found at radio wavelengths. We attribute the detected I-band periodicities to the periods of rotation of the dwarfs, supported by radius estimates and measured values for the objects. Based on the detected period of rotation in the I band, along with confirmation of strong magnetic fields from recent radio observations, we argue for magnetically induced spots as the cause of this periodic variability. The I-band rotational modulation of the L3.5 dwarf 2MASS J00361617+1821104 appeared to vary in amplitude with time. We conclude that the most likely cause of the I-band variability for this object is magnetic spots, possibly coupled with time-evolving features such as dust clouds.
Document Details
- Document Type
- Technical Report
- Publication Date
- Oct 20, 2007
- Accession Number
- ADA477306
Entities
People
- A. Antonova
- A. Golden
- F. J. Vrba
- G. Hallinan
- H. Clifford Lane
- J. G. Doyle
- R. F. Butler
- R. P. Boyle
- Robert T. Zavala
- S. Bourke
Organizations
- United States Naval Observatory Flagstaff Station