The Disk Substructures at High Angular Resolution Project (DSHARP). IX. A High-definition Study of the HD 163296 Planet-forming Disk

The Atacama Large Millimeter/submillimeter Array observations of protoplanetary disks acquired by the Disk Substructure at High Angular Resolution Project resolve the dust and gas emission on angular scales as small as 3 astronomical units, offering an unprecedented detailed view of the environment...

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Veröffentlicht in:	Astrophysical journal. Letters 2018-12, Vol.869 (2), p.L49
Hauptverfasser:	Isella, Andrea, Huang, Jane, Andrews, Sean M., Dullemond, Cornelis P., Birnstiel, Tilman, Zhang, Shangjia, Zhu, Zhaohuan, Guzmán, Viviana V., Pérez, Laura M., Bai, Xue-Ning, Benisty, Myriam, Carpenter, John M., Ricci, Luca, Wilner, David J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Angular resolution Asymmetry Celestial bodies Continuum radiation Dust Dust emission Emissions High definition Optical analysis Optical thickness Planet formation planet-disk interactions Planets Protoplanetary disks Protoplanets Radio telescopes Sciences of the Universe Spatial resolution Substructures techniques: interferometric
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