Results 111 to 120 of about 16,676 (207)

Shadow-induced Warps in Protoplanetary Disks

open access: yesThe Astrophysical Journal Letters
Shadows are commonly observed in protoplanetary disks in near-infrared (NIR) and (sub)millimeter images, often cast by misaligned inner disks or other obscuring material.
Shangjia Zhang   +2 more
doaj   +1 more source

<i>Herschel</i> survey and modelling of externally-illuminated photoevaporating protoplanetary disks. [PDF]

open access: yesAstron Astrophys, 2017
Champion J   +7 more
europepmc   +1 more source

SO Emission in the Dynamically Perturbed Protoplanetary Disks around CQ Tau and MWC 758

open access: yesThe Astrophysical Journal
We report the serendipitous detection of the SO J _N  = 6 _5 –5 _4 (219.949 GHz) rotational transition in archival Atacama Large Millimeter/submillimeter Array observations of the spiral hosting protoplanetary disks around CQ Tau (with ≈4.9 σ ...
Francesco Zagaria   +27 more
doaj   +1 more source

Chemistry in Protoplanetary Disks

open access: yes, 2010
14 pages, 2 figures, 2 tables, pre-final chapter to be published in Encyclopedia of Astrobiology by Gargaud, M.; Cernicharo, J.; Viso, M.; Cleaves II, H.J.; Pinti, D.; Amils, R.; Kobayashi, K.; Irvine, W.M. (Eds.), Springer, 2011 (ISBN: 978-3-642-11279-9)
openaire   +2 more sources

Observability of Substructures in the Planet-forming Disk in the (Sub)centimeter Wavelength with SKA and ngVLA

open access: yesThe Astrophysical Journal
Current imaging observations of protoplanetary disks using the Atacama Large Millimeter/submillimeter Array (ALMA) primarily focus on the submillimeter wavelength, leaving a gap in effective observational approaches for centimeter-sized dust, which is ...
Yinhao Wu   +3 more
doaj   +1 more source

Dust traps in protoplanetary disks efficiently form organic macromolecular matter

open access: yes, 2023
Ligterink N   +6 more
europepmc   +1 more source

PROTOPLANETARY DISK EVOLUTION

open access: yes, 2004
One of the most active fields of research in accretion disk theory is understanding the mechanisms that transport angular momentum outward. Two instabilities are thought to be responsible for it in massive, magnetized disks: the magnetorotational instability (MRI) caused by the presence of a weak magnetic field, and gravitational instabilities.This PhD
openaire   +1 more source

Molecular Gas Tracers in Young and Old Protoplanetary Disks

open access: yesThe Astrophysical Journal
Molecular emission is used to investigate both the physical and chemical properties of protoplanetary disks. Therefore, to derive disk properties accurately, we need a thorough understanding of the behavior of the molecular probes upon which we rely ...
Dana E. Anderson   +8 more
doaj   +1 more source

Chemistry in Protoplanetary Disks

open access: yesReviews in Mineralogy and Geochemistry
Chapter 2 accepted for publication in the Reviews in Mineralogy and Geochemistry (RiMG) Volume 90 on "Exoplanets: Compositions, Mineralogy, and Evolution" edited by Natalie Hinkel, Keith Putirka, and Siyi Xu; 24 pages and 4 ...
openaire   +2 more sources

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