Ultraviolet spectroscopy of the hotspot in the classical T Tauri star DI Cep: Observational indications of magnetically channelled accretion

Monthly Notices of the Royal Astronomical Society

Volumn 283, Issue 1, 1996, Pages 55-65

  Gómez de Castro, Ana I ^a   Fernández, Matilde ^b  

^a UNIVERSIDAD COMPLUTENSE DE MADRID   (Spain)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

Stars: activity; Stars: formation; Stars: individual: DI Cep; Stars: magnetic field; Stars: pre main sequence; Ultraviolet: stars

Indexed keywords

CHROMOPHORES; MAGNETIC FIELDS; SILICON COMPOUNDS; ULTRAVIOLET SPECTROSCOPY;

HOTSPOTS; STAR: ACTIVITY; STAR: INDIVIDUAL: DI CEP; STARS FORMATION; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: MAGNETIC FIELD; STARS: PRE-MAIN SEQUENCE; T TAURI STARS; ULTRAVIOLET: STARS; UV SPECTRUM;

STARS;

EID: 0039080569     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/283.1.55     Document Type: Article

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