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Encyclopedia of Astrobiology, 2021
Jonathan P. Williams, M. Hogerheijde
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Jonathan P. Williams, M. Hogerheijde
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A circumbinary protoplanetary disk in a polar configuration
Nature Astronomy, 2019Nearly all young stars are initially surrounded by ‘protoplanetary’ disks of gas and dust, and in the case of single stars at least 30% of these disks go on to form planets1.
G. Kennedy+8 more
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Protostars and Protoplanetary Disks [PDF]
A great wealth of observational information about young stars has been obtained at infrared and longer wavelengths in the last decade. Combined with continued theoretical progress, these observations have pushed our understanding of the overall star formation process to a satisfying level.
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Constraining Gas-phase Carbon, Oxygen, and Nitrogen in the IM Lup Protoplanetary Disk
Astrophysical Journal, 2018We present new constraints on gas-phase C, N, and O abundances in the molecular layer of the IM Lup protoplanetary disk. Building on previous physical and chemical modeling of this disk, we use new ALMA observations of C2H to constrain the C/O ratio in ...
L. Cleeves+9 more
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Protoplanetary Disk, Chemistry
2011▶ Protoplanetary disks (PPDs) surrounding young stars are short-lived (~1–10 Myr), compact (~10–1,000 AU) rotating reservoirs of gas and dust. Disks are believed to be the birthplaces of planetary systems, where tiny grains are assembled into pebbles,▶ planetesimals, and eventually planets, asteroids, and comets.
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The partitioning of the inner and outer Solar System by a structured protoplanetary disk
Nature Astronomy, 2020R. Brasser, S. Mojzsis, S. Mojzsis
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Protostellar and Protoplanetary Disks [PDF]
It is barely a decade since the first molecular line images of disks around embedded and pre-main sequence stars were published (Beckwith et al., 1986; Mundy et al., 1986; Sargent & Beckwith 1987). In the intervening years there has been steady progress in detecting and analyzing these disks, which are an expected by-product of the star formation ...
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