tailieunhanh - The protoplanetary disc HD 163296 as observed by ALMA

HD 163296 is one of the few protoplanetary discs displaying rings in the dust component. The present work uses ALMA observations of the mm continuum emission, which have significantly better spatial resolution (~8 au) than previously available, to provide new insight into the morphology of the dust disc and its double ring structure. The disc is shown to be thin, and its position angle and inclination with respect to the sky plane are accurately measured as are the locations and shapes that characterise the observed ring-gap structure. Significant modulation of the intensity of the outer ring emission is revealed and discussed. In addition, earlier ALMA observations of the emission of three molecular lines, CO(2-1), C18O(2-1), and DCO+ (3-2) with a resolution of ~70 au are used to demonstrate the Keplerian motion of the gas, which is found to be consistent with a central mass of solar masses. An upper limit of ~9% of the rotation velocity is placed on the in-fall velocity. The beam size is shown to give the dominant contribution to the line widths, accounting for both their absolute values and their dependence on the distance to the central star. | Doi 2 .03-16 PHYSICAL SCIENCES PHYSICS The protoplanetary disc HD 163296 as observed by ALMA . Diep . Hoai . Ngoc . Nhung . Phuong . Thai and P. Tuan-Anh Department of Astrophysics Vietnam National Space Center Vietnam Academy of Science and Technology Received 25 February 2019 accepted 3 April 2019 Abstract HD 163296 is one of the few protoplanetary discs displaying rings in the dust component. The present work uses ALMA observations of the mm continuum emission which have significantly better spatial resolution 8 au than previously available to provide new insight into the morphology of the dust disc and its double ring structure. The disc is shown to be thin and its position angle and inclination with respect to the sky plane are accurately measured as are the locations and shapes that characterise the observed ring-gap structure. Significant modulation of the intensity of the outer ring emission is revealed and discussed. In addition earlier ALMA observations of the emission of three molecular lines CO 2-1 C18O 2-1 and DCO 3-2 with a resolution of 70 au are used to demonstrate the Keplerian motion of the gas which is found to be consistent with a central mass of solar masses. An upper limit of 9 of the rotation velocity is placed on the in-fall velocity. The beam size is shown to give the dominant contribution to the line widths accounting for both their absolute values and their dependence on the distance to the central star. Keywords planetary systems protoplanetary discs submillimetre astronomy. Classification number Corresponding author Email pndiep@ Introduction The study of ring-like structures observed in the dust emission of protoplanetary discs is expected to shed light on the mechanisms governing the formation of planets. Only two such discs were known before the discovery of the ring-gap structure of the HD 163296 disc 1 TW Hya 2 and HL Tau 3 . Although still being debated such ringgap .

• Địa Lý
• Planetary systems
• Protoplanetary discs
• Submillimetre astronomy
• Observed by ALMA
• The protoplanetary disc HD 163296