Recurring millimeter flares as evidence for star-star magnetic reconnection events in the DQ Tauri PMS binary system

Astronomy and Astrophysics

Volumn 521, Issue 4, 2010, Pages

  Salter, D M ^a   Kospal A ^a   Getman, K V ^b   Hogerheijde, M R ^a   Van Kempen, T A ^c   Carpenter, J M ^d   Blake, G A ^e   Wilner, D ^c  

^a LEIDEN UNIVERSITY   (Netherlands)

^b PENNSYLVANIA STATE UNIVERSITY   (United States)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

binaries: spectroscopic; radio continuum: stars; stars: flare; Stars: individual: DQ Tau; stars: magnetic field; stars: pre main sequence

Indexed keywords

BINARIES: SPECTROSCOPIC; RADIO CONTINUUM: STARS; STARS: FLARE; STARS: INDIVIDUAL: DQ TAU; STARS: MAGNETIC FIELD; STARS: PRE-MAIN SEQUENCE;

ASTROPHYSICS; GEOPHYSICS; MAGNETIC FIELD EFFECTS; MAGNETISM; MAGNETOSPHERE; POLARIZATION; SPECTROSCOPY; SYNCHROTRONS;

STARS;

EID: 77958075276     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015197     Document Type: Article

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