Mass Loss in Be Stars: News from Two Fronts
GalaxiesBe stars are characterized by the presence of a circumstellar Keplerian disk formed from material ejected from the rapidly rotating stellar surface.
Alex C. Carciofi +7 more
doaj +1 more source
Unveiling Su Aurigae in the near Infrared: New high spatial resolution results using Adaptive Optics
, 2004 We present here new results on circumstellar nebulosity around SU Aurigae, a T-Tauri star of about 2 solar mass and 5 Myrs old at 152 pc in the J, H and K bands using high resolution adaptive optics imaging (0$\farcs$30) with the Penn state IR Imaging ...
Abhijit Chakraborty +5 more
core +2 more sources
Disk in the Circumstellar Envelope of Carbon Mira V Cygni
The Astronomical JournalAsymptotic giant branch (AGB) stars are the primary source of dust and complex molecules in the interstellar medium. The determination of outflow parameters is often hindered by the unknown geometry of the circumstellar environment, creating a demand for
Boris S. Safonov +4 more
doaj +1 more source
The effect of local optically thick regions in the long-wave emission of young circumstellar disks [PDF]
, 2012 Luca Ricci +5 more
openalex +3 more sources
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
Using the Coolest Ae Stars to Constrain Circumstellar Disk Viscosity
The Astrophysical JournalClassical 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
Photometric Monitoring of the First Eclipsing Binary Be Star: V658 Car
GalaxiesV658 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
The evolution of dust in the terrestrial planet region of circumstellar disks around young stars.
, 2021 D. Dutkevitch
openalex +2 more sources
Light Echoes of Time-resolved Flares and Application to Kepler Data
The Open Journal of AstrophysicsLight 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
Detection of the Circumstellar Disk Associated with 2MASS J0820-8003 in the eta Cha Cluster
, 2012 The Nearby Young Moving Groups (NYMGs) of stars are ideal for the study of evolution circumstellar disks in which planets may form because their ages range from a few Myr to about 100 Myr, about the same as the interval over which planets are thought to ...
Constantin, Ana-Maria +3 more
core +1 more source