Modelling the radio pulses of an ultracool dwarf

Astronomy and Astrophysics

Volumn 525, Issue 17, 2011, Pages

  Yu, S ^a   Hallinan, G ^b,c   Doyle, J G ^a   MacKinnon, A L ^d   Antonova, A ^e   Kuznetsov, A ^a,f   Golden, A ^b   Zhang, Z H ^g  

^a ARMAGH OBSERVATORY   (United Kingdom)

^b NATIONAL UNIVERSITY OF IRELAND   (Ireland)

^c UNIVERSITY OF CALIFORNIA   (United States)

^d UNIVERSITY OF GLASGOW   (United Kingdom)

^e UNIVERSITY OF SOFIA   (Bulgaria)

^f INSTITUTE OF SOLAR TERRESTRIAL PHYSICS   (Russian Federation)

^g UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

Author keywords

brown dwarfs; magnetic fields; masers; polarization; radio continuum: stars; stars: low mass

Indexed keywords

CYCLOTRON RADIATION; CYCLOTRONS; ELECTROMAGNETIC WAVE POLARIZATION; LUMINANCE; MAGNETIC FIELDS; MAGNETOSPHERE; MASERS; POLARIZATION; STARS; TOPOLOGY; X RAYS;

AMPLIFICATION MECHANISM; BROWN DWARFS; ELECTRON CYCLOTRON MASER INSTABILITY; HIGH DEGREE OF VARIABILITY; HIGH FREQUENCY ELECTROMAGNETIC WAVES; RADIO CONTINUUM: STARS; STARS: LOW MASS; SURFACE MAGNETIC FIELD;

MAGNETOPLASMA;

EID: 79951471697     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015580     Document Type: Article

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