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Dusty Blue Supergiants: News from High-Angular Resolution Observations
An overview is presented of the recent advances in understanding the B[e] phenomenon among blue supergiant stars in light of high-angular resolution observations and with an emphasis on the results obtained by means of long baseline optical stellar ...
W. J. de Wit +2 more
doaj +1 more source
Submillimetre observations of circumstellar dust
Bibliography: p. 113-120.
openaire +2 more sources
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley +1 more source
Recent Atacama Large Millimeter/submillimeter Array (ALMA) observations with 0 $\mathop{.}\limits^{^{\prime\prime} }$ 1 resolution have revealed characteristic substructures in circumstellar disks around young Class I sources, providing clues to the ...
Ayumu Shoshi +6 more
doaj +1 more source
Dust distribution in circumstellar disks harboring multi-planet systems
Context. Theoretical formation models and exoplanet detection surveys indicate that systems with multiple giant planets are common. Aims. We investigate how multiple super-thermal-mass planets embedded in a circumstellar disk shape the dust distribution ...
Roatti V., Picogna G., Marzari F.
doaj +1 more source
Dust dynamics in planet-forming discs in binary systems. [PDF]
Zagaria F +3 more
europepmc +1 more source
Hydrodynamical models and synthetic spectra of circumstellar dust shells around AGB stars. Pt. 1 Stationary solutions [PDF]
We present a sample of hydrodynamical steady state models of circumstellar gas/dust shells around late type giants together with computed spectral energy distributions (SEDs).
Kiel Univ. (Germany). Inst. fuer Astronomie und Astrophysik) +6 more
core
Deep Search for a Scattered Light Dust Halo Around Vega with the Hubble Space Telescope
We present a provisory scattered-light detection of the Vega debris disk using deep Hubble Space Telescope (HST) coronagraphy (PID 16666). At only 7.7 pc, Vega is immensely important in debris disk studies both for its prominence and also because it ...
Schuyler G. Wolff +8 more
doaj +1 more source
(Sub)millimeter dust polarization in protoplanetary disks has revealed the presence of large (∼100 μ m) dust grains that are aligned along their long axis following the azimuthal direction of the disk.
Zhe-Yu Daniel Lin +10 more
doaj +1 more source
Probing Dust and Gas Properties Using Ringed Disks
How rapidly a planet grows in mass and how far it may park from the host star depend sensitively on two nondimensional parameters: Stokes number St and turbulent α .
Eve J. Lee
doaj +1 more source

