Results 81 to 90 of about 2,036 (233)

Using the Coolest Ae Stars to Constrain Circumstellar Disk Viscosity

open access: yesThe Astrophysical Journal
Classical Ae (CAe) stars are main-sequence, A-type stars with H α emission but no signature of dust. They are thought to be the cool extension of the classical Be stars to lower masses.
R. Anusha, T. A. A. Sigut
doaj   +1 more source

The Disks In Scorpius–Centaurus Survey (DISCS). I. Four Newly Resolved Debris Disks in Polarized Intensity Light

open access: yesThe Astronomical Journal
The presence of infrared excesses around stars directly correlates with spatially resolved imaging detections of circumstellar disks at both millimeter and optical/near-infrared wavelengths.
Justin Hom   +10 more
doaj   +1 more source

Light Echoes of Time-resolved Flares and Application to Kepler Data

open access: yesThe Open Journal of Astrophysics
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

Photometric Monitoring of the First Eclipsing Binary Be Star: V658 Car

open access: yesGalaxies
V658 Car is the first known eclipsing binary system involving a classical Be star and an sdOB companion, offering a unique opportunity to study disk physics and binary interactions in unprecedented detail. From TESS data and multi-color observations from
Tajan H. de Amorim   +11 more
doaj   +1 more source

87th Annual Meeting of the Meteoritical Society 2025: Abstracts

open access: yes
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley   +1 more source

WISEDETECTION OF THE CIRCUMSTELLAR DISK ASSOCIATED WITH 2MASS J0820-8003 IN THE η Cha CLUSTER [PDF]

open access: green, 2012
M. Simon   +3 more
openalex   +1 more source

Cloud Dissipation and Disk Wind in the Late Phase of Star Formation

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

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