High-resolution visible spectroscopy of the jet-driving star Th 28 *

Astronomy and Astrophysics

Volumn 511, Issue 1, 2010, Pages

  Comeron F ^a   Fernandez M ^b  

^a EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^b INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

Author keywords

Stars: formation; Stars: individual: Th 28, Sz 102, Krautter's star; Stars: mass loss; Stars: pre main sequence

Indexed keywords

DISKS (STRUCTURAL COMPONENTS); ELECTROMAGNETIC WAVE EMISSION; INFRARED SPECTROPHOTOMETERS; JETS; MAGNETOSPHERE; ROTATING DISKS; ROTATION;

ACCRETION FLOW; ACCRETION RATE; BASIC PARAMETERS; CENTRAL SOURCE; DRIVING SOURCE; EMISSION LINES; EQUIVALENT WIDTH; FORBIDDEN LINES; HERBIG-HARO OBJECTS; HIGH RESOLUTION; RADIAL VELOCITY; RED-SHIFTED; SPECTRUM DISPLAYS; STARS: FORMATION; STARS: MASS-LOSS; STARS: PRE-MAIN SEQUENCE; STARS:FORMATION-STARS; STELLAR WIND; STRUCTURAL COMPONENT; T TAURI STARS; THIRD COMPONENT; VISIBLE EMISSIONS; VISIBLE SPECTROSCOPY; YOUNG STELLAR OBJECTS;

STARS;

EID: 77249124849     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912959     Document Type: Article

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