作者: Á. Sánchez-Monge , R. Cesaroni , M. T. Beltrán , M. S. N. Kumar , T. Stanke
DOI: 10.1051/0004-6361/201321134
关键词: Star formation 、 Circumbinary planet 、 Stellar mass 、 Binary system 、 Astronomy 、 Central mass 、 Accretion (astrophysics) 、 Vector field 、 Physics 、 Astrophysics 、 Overtone
摘要: We report on ALMA observations of continuum and molecular line emission with 0 ''.4 resolution towards the high-mass star-forming region G35.20-0.74 N. Two dense cores are detected in typical hot-core tracers (e. g., CH3CN) that reveal velocity gradients. In one these cores, field can be fitted an almost edge-on Keplerian disk rotating about a central mass similar to 18 M-circle dot. This finding is consistent results recent study CO first overtone bandhead at 2.3 mu m The radius greater than or 2500 au 3 To reconcile observed bolometric luminosity (similar 3x10(4) L-circle dot) estimated stellar dot, we propose latter total binary system.