Evidence for high accretion rates in weak-line T Tauri stars?

Monthly Notices of the Royal Astronomical Society

Volumn 347, Issue 3, 2004, Pages 937-941

  Littlefair, S P ^a   Naylor, Tim ^a   Harries, Tim J ^a   Retter, Alon ^b   O'Toole, S ^b,c  

^a UNIVERSITY OF EXETER   (United Kingdom)

^b UNIVERSITY OF SYDNEY   (Australia)

^c UNIVERSITY OF ERLANGEN NUREMBERG   (Germany)

Author keywords

Accretion, accretion discs; Instabilities; Planetary systems: protoplanetary discs; Stars: dwarf novae; Stars: pre main sequence

Indexed keywords

MASS TRANSFER;

ACCRETION RATE; ACCRETION: ACCRETION DISKS; COMPOSITE SPECTRA; HΑ EMISSION; PLANETARY SYSTEMS:PROTOPLANETARY DISKS; SPECTRAL TYPES; STARS: DWARF NOVAE; STARS: PRE-MAIN SEQUENCE; T TAURI STARS; WEAK LINES;

STARS;

EID: 1642518324     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07263.x     Document Type: Article

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