The evolution of dust in the terrestrial planet region of circumstellar disks around young stars.
D. Dutkevitch
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Light Echoes of Time-resolved Flares and Application to Kepler Data
Light echoes of stellar flares provide an intriguing option for exploring protoplanetary disks in young stellar systems. Previous work on light echoes of circumstellar disks made use of delta-function flares for modeling.
Austin King, Benjamin C. Bromley
doaj +1 more source
High-Resolution Near-Infrared Polarimetry of a Circumstellar Disk around UX Tau A [PDF]
Ryoko Tanii +67 more
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Phosphorus-bearing molecules PO and PN at the edge of the Galaxy. [PDF]
Koelemay LA, Gold KR, Ziurys LM.
europepmc +1 more source
Cloud Dissipation and Disk Wind in the Late Phase of Star Formation
We perform a long-term simulation of star and disk formation using three-dimensional nonideal magnetohydrodynamics. The simulation starts from a prestellar cloud and proceeds through the long-term evolution of the circumstellar disk until ∼1.5 × 10 ^5 yr
Masahiro N. Machida, Shantanu Basu
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Questing for Minute Traces of Molecular Gas in Circumstellar Debris Disks: AU Microscopii and 49 Ceti Edition [PDF]
Zachary Stafford Lambros
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GANBISS: a new GPU accelerated N-body code for binary star systems. [PDF]
Zimmermann M, Pilat-Lohinger E.
europepmc +1 more source
The discovery of protoplanets and circumplanetary disks provides a unique opportunity to characterize planet formation through observations. Massive protoplanets shape the physical and chemical structure of their host circumstellar disk by accretion ...
Felipe Alarcón, Edwin A. Bergin
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Reference Star Differential Imaging of Close-in Companions and Circumstellar Disks with the NIRC2 Vortex Coronagraph at the W. M. Keck Observatory [PDF]
Garreth Ruane +13 more
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Identification of Possible Stellar Companions via Speckle Interferometry in a Sample of Be Stars II
This study investigates the identification of possible stellar companions in a sample of Be stars using speckle interferometry. Be stars, which are rapidly rotating B-type stars exhibiting emission lines due to the presence of circumstellar disks, have ...
C. A. Guerrero +3 more
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