Results 141 to 150 of about 71,588 (268)

Resolving Molecular Line Emission from Protoplanetary Disks: Observational Prospects for Disks Irradiated by Infalling Envelopes [PDF]

, 2000
José F. Gómez, Paola D’Alessio
openalex   +1 more source

Asymmetric Temperature Variations In Protoplanetary Disks. I. Linear Theory, Corotating Spirals, and Ring Formation

The Astrophysical Journal
Protoplanetary disks can exhibit asymmetric temperature variations due to phenomena such as shadows cast by the inner disk or localized heating by young planets. We investigate the disk features induced by these asymmetric temperature variations. We find
Zhaohuan Zhu, Shangjia Zhang, Ted M. Johnson   +2 more
doaj   +1 more source

Magnetorotational Instability in Protoplanetary Disks. II. Ionization State and Unstable Regions [PDF]

, 2000
Takayoshi Sano, Shoken M. Miyama, Toyoharu Umebayashi, Takenori Nakano   +3 more
openalex   +1 more source

Gap Formation in the Dust Layer of 3D Protoplanetary Disks

, 2007
We numerically model the evolution of dust in a protoplanetary disk using a two-phase (gas+dust) Smoothed Particle Hydrodynamics (SPH) code, which is non-self-gravitating and locally isothermal. The code follows the three dimensional distribution of dust
A. Crida, A.J. Weinberger, D.N.C. Lin, G. Bryden, G. Schneider, H. Beust, J. Papaloizou, J.-F. Gonzalez, L. Barrière-Fouchet, L. Fouchet, M. Val-Borro de, N. Calvet, N.I. Shakura, P. Varnière, R. Alexander, S. T. Maddison, S. Wolf, S.-J. Paardekooper, V. Piétu, W. Kley, W.K.M. Rice, W.K.M. Rice   +21 more
core   +2 more sources

The Importance of Photoprocessing in Protoplanetary Disks [PDF]

, 2000
Karen Willacy, W. D. Langer
openalex   +1 more source

Planetesimal formation by the streaming instability in a photoevaporating disk

, 2017
Recent years have seen growing interest in the streaming instability as a candidate mechanism to produce planetesimals. However, these investigations have been limited to small-scale simulations. We now present the results of a global protoplanetary disk
Carrera, Daniel, Davies, Melvyn B., Gorti, Uma, Johansen, Anders   +3 more
core   +1 more source

Insight into the Formation of β Pic b through the Composition of Its Parent Protoplanetary Disk as Revealed by the β Pic Moving Group Member HD 181327

The Astronomical Journal
It has been suggested that β Pic b has a supersolar metallicity and subsolar C/O ratio. Assuming solar carbon and oxygen abundances for the star β Pic and therefore the planet’s parent protoplanetary disk, β Pic b’s C/O ratio suggests that it formed via ...
Henrique Reggiani, Jhon Yana Galarza, Kevin C. Schlaufman, David K. Sing, Brian F. Healy, Andrew McWilliam, Joshua D. Lothringer, Laurent Pueyo   +7 more
doaj   +1 more source

Fully compressible simulations of the baroclinic instability in protoplanetary disks

EPJ Web of Conferences, 2013
The occurrence of the baroclinic instability in protoplanetary disks is investigated using fully compressible numerical simulations. We study the role of disk stratification and heat transfer in the development of the instability. Vortices are found to
Barge Pierre, Richard Samuel
doaj   +1 more source

The Formation and Role of Vortices in Protoplanetary Disks [PDF]

, 2000
Patrick Godon, Mario Livio
openalex   +1 more source

Debris Disks: Probing Planet Formation

, 2018
Debris disks are the dust disks found around ~20% of nearby main sequence stars in far-IR surveys. They can be considered as descendants of protoplanetary disks or components of planetary systems, providing valuable information on circumstellar disk ...
A Bonsor, A Bonsor, A Bonsor, A Brandeker, A Gáspár, A Gáspár, A Hardy, A Moro-Martín, A Moór, A Schneider, A Shannon, A Shannon, AJ Mustill, AJ Mustill, AJW Richert, AM Hughes, AM Hughes, AM Lagrange, AP Jackson, AP Jackson, AV Krivov, AV Krivov, AV Krivov, B Ercolano, B Mennesson, B Sibthorpe, BP Bowler, C Eistrup, C Schüppler, C Vitense, CC Stark, Christine H. Chen, CM Lisse, CM Telesco, D Carrera, D Li, D Tamayo, DA Fischer, DA Golimowski, E Chiang, EJ Lee, ER Nesvold, ER Nesvold, F Geiler, F. Kiefer, G Bryden, GM Kennedy, GM Kennedy, GM Kennedy, H Beust, H Beust, H Genda, HF Levison, HYA Meng, HYA Meng, HYA Meng, J Lieman-Sifry, J Péricaud, J Wisdom, J. Olofsson, JC Augereau, JH Rhee, JM Carpenter, JN Winn, JS Greaves, JS Greaves, K Heng, KYL Su, L Matrà, L Matrà, L Matrà, L Ricci, LA Cieza, LE Strubbe, M Booth, M Booth, M Pan, MA MacGregor, MA MacGregor, MA Muñoz-Gutiérrez, Maryam Tabeshian, MC Wyatt, MC Wyatt, MC Wyatt, MC Wyatt, MC Wyatt, MC Wyatt, MC Wyatt, MC Wyatt, MC Wyatt, MC Wyatt, MC Wyatt, MC Wyatt, MC Wyatt, MC Wyatt, N Kains, N Pawellek, NA Kaib, ND Thureau, NM Phillips, O Panić, P Faber, P Kalas, P Thébault, Q Kral, Q Kral, Q. Kral, R Smith, S Marino, S Marino, S Marino, S Rappaport, S. Krijt, SJ Kenyon, SJ Kenyon, SJ Kenyon, SJ Kenyon, SN Raymond, T Currie, T Löhne, T Löhne, T Takeuchi, TD Pearce, TD Pearce, TS Boyajian, V Faramaz, W Lyra, WRF Dent, X Zheng, Y Hasegawa, Á Kóspál, É Morey   +131 more
core   +1 more source