Large Fluctuations within 1 au in Protoplanetary Disks
The Astrophysical JournalProtoplanetary disks are often assumed to change slowly and smoothly during planet formation. Here, we investigate the time evolution of isolated disks subject to viscosity and a disk wind. The viscosity is assumed to increase rapidly at around 900 K due
John Chambers
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The Astrophysical JournalWe present JWST broadband images of the highly inclined protoplanetary disk SSTc2d J163131.2-242627 (Oph163131) from 2.0 to 21 μ m. The images show a remarkable evolution in disk structure with wavelength, quite different from previous JWST observations ...
Marion Villenave +8 more
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Modeling the Impact of Moderate External UV Irradiation on Disk Chemistry
The Astrophysical JournalThe chemistry within a protoplanetary disk is greatly affected by external radiation from the local stellar environment. Previous work has focused on extreme radiation fields, representative of the center of something like the Orion Nebula Cluster ...
Rachel E. Gross, L. Ilsedore Cleeves
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Evolution of the Solar Nebula. III. Protoplanetary Disks Undergoing Mass Accretion [PDF]
, 1997 Alan P. Boss
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A numerical turbulence model for multiphase flows in the protoplanetary nebula [PDF]
, 1995 Joëlle M. Champney +2 more
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A Comparison of Presolar Isotopic Signatures in Laboratory-Studied Primitive Solar System Materials and Comet 67P/Churyumov-Gerasimenko: New Insights from Light Elements, Halogens, and Noble Gases. [PDF]
Space Sci Rev, 2023 Hoppe P, Rubin M, Altwegg K.
europepmc +1 more source
Molecular Line Observations of the Protoplanetary Nebula, IRAS 19312+1950 [PDF]
, 2003 Shuji Deguchi, Jun‐ichi Nakashima
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86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page i-xlii, August 2024.
wiley +2 more sources
The Astrophysical JournalThe most powerful stellar flares driven by magnetic energy occur during the early pre-main-sequence (PMS) phase. The Orion Nebula represents the nearest region populated by young stars, showing the greatest number of flares accessible to a single ...
Konstantin V. Getman +10 more
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Thermal and hydrostatic structure of the protoplanetary nebula exposed to stellar radiation and stellar wind from the central star [PDF]
, 2007 Young Seok Yun +2 more
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