Mapping radio emitting-region on low-mass stars and brown dwarfs
Strong magnetic activity in ultracool dwarfs (UCDs, spectral classes later than M7) have emerged from a number of radio observations, including the periodic beams. The highly (up to 100%) circularly polarized nature of the emission point to an effective amplification mechanism of the high-frequency...
Main Authors: | Hallinan G., Yu S., Doyle J.G., MacKinnon A.L. |
---|---|
Format: | Article |
Language: | English |
Published: |
EDP Sciences
2011-07-01
|
Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/20111606013 |
Similar Items
-
The study of low-mass stars and brown dwarfs
by: Cossburn, Martin R.
Published: (1999) -
Low-mass stars and brown dwarfs : optical/infrared photometry and spectroscopy of low-mass stars and brown dwarfs in the Field and Young Clusters
by: King, Robert R.
Published: (2009) -
Low mass stars and brown dwarfs in open clusters
by: Pinfield, David J.
Published: (1998) -
Photometry and spectroscopy of low mass stars and brown dwarfs
by: Steele, Iain A.
Published: (1994) -
Low mass stars and brown dwarfs around σ Orionis
by: Kenyon, Michael John
Published: (2004)