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Protostars and Protoplanetary Disks

Astrophysics and Space Science, 1997
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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Protoplanetary Disk

2021
Jonathan P. Williams   +1 more
openaire   +1 more source

Protoplanetary disk structure

2009
Planets form from protoplanetary disks of gas and dust that are observed to surround young stars for the first few million years of their evolution. Disks form because stars are born from relatively diffuse gas (with particle number density n ~ 10 5 cm −3 ) that has too much angular momentum to collapse directly to stellar densities ( n ~ 10 24 cm
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Protoplanetary Disk Chemistry

Annual Review of Astronomy and Astrophysics, 2023
Karin Öberg, Stefano Facchini
exaly  

Protoplanetary Disks

2003
I. De Gregorio-Monsalvo   +2 more
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H2O in Protoplanetary Disks

2013
Protoplanetary disks represent the stage between the pre-stellar collapse of the molecolar cloud and the formation of a planetary system surrounding a main sequence star. The goal of the DIANA FP7 project (P.I.: P.Woitke) is to investigate the disks in multiwavelengths, considering available data of photometry and spectroscopy, and give reason of the ...
Antonellini, Stefano   +3 more
openaire   +1 more source

A JWST inventory of protoplanetary disk ices

Astronomy and Astrophysics, 2023
Ardjan Sturm, M K McClure, A C A Boogert
exaly  

Observations of edge-on protoplanetary disks with ALMA

Astronomy and Astrophysics, 2020
Gerrit van der Plas   +2 more
exaly  

A simple model for the evolution of the dust population in protoplanetary disks

Astronomy and Astrophysics, 2012
Tilman Birnstiel, Hubert Klahr
exaly  

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