Results 21 to 30 of about 1,969,695 (207)

Microlensing of circumstellar envelopes: II. emission lines from radial and azimuthal flow during fold caustic crossings [PDF]

open access: yes, 2003
This paper examines the line profile evolution due to bulk motion in circumstellar envelopes during microlensing fold caustic crossing events. These events have recently been shown to be a sensitive probe of stellar surface brightness profiles, thus ...
Bryce, H.M.   +5 more
core   +1 more source

Hot Gas in the Circumstellar Bubble S308 [PDF]

open access: yesThe Astrophysical Journal, 2003
18 pages, 3 figures, to appear in the Astrophysical Journal, Dec 20 ...
Chu, Y. -H.   +4 more
openaire   +2 more sources

Microlensing of circumstellar envelopes III. Line profiles from stellar winds in homologous expansion [PDF]

open access: yes, 2006
This paper examines line profile evolution due to the linear expansion of circumstellar material obsverved during a microlensing event. This work extends our previous papers on emission line profile evolution from radial and azimuthal flow during point ...
Bryce, H.M.   +8 more
core   +1 more source

Detection of circumstellar gas associated with GG Tauri

open access: yesThe Astrophysical Journal, 1993
Double-peaked (C-12)O (1-0) emission centered on the young T Tauri star GG Tau possesses a line profile which may be modeled on the assumption that CO emission arises in an extended circumstellar disk. While bounds on the observed gas mass can be estimated on this basis, it is suggested that a large amount of mass could lie within a small and optically
SKRUTSKIE, MF   +8 more
openaire   +2 more sources

Dust Rings in the Circumstellar Gas Disks [PDF]

open access: yesSymposium - International Astronomical Union, 2004
In optically thin gas disks around young Vega-type stars, dust grains are exposed to the stellar radiation pressure and gas drag force. The combination of these forces pushes the grains away from the central star. Typically, 10–100 μm grains migrate outward to become concentrated at the outer edge of the gas disk.
Taku Takeuchi, Pawel Artymowicz
openaire   +1 more source

Infrared Spectroscopy of U Equulei’s Warm Circumstellar Gas [PDF]

open access: yesThe Astrophysical Journal, 2005
21 pages incl.
Geballe, T. R.   +3 more
openaire   +2 more sources

Sustained Kozai–Lidov Oscillations in Misaligned Circumstellar Gas Disks [PDF]

open access: yesThe Astrophysical Journal Letters, 2021
Abstract A disk around one component of a binary star system with sufficiently high inclination can undergo Kozai–Lidov (KL) oscillations during which the disk inclination and disk eccentricity are exchanged. Previous studies show that without a source of accretion, KL unstable disks exhibit damped oscillations, due to viscous ...
Jeremy L. Smallwood   +2 more
openaire   +2 more sources

Debris Disks around Nearby Stars with Circumstellar Gas [PDF]

open access: yesThe Astrophysical Journal, 2008
10 pages including 4 figures.
Roberge, Aki, Weinberger, Alycia J.
openaire   +2 more sources

Evolution of Gas and Dust in Circumstellar Disks [PDF]

open access: yesSymposium - International Astronomical Union, 2000
A clear understanding of the chemical processing of matter as it is transferred from a molecular cloud to a planetary system depends heavily on the physical conditions endured by gas and dust as these accrete onto a disk and are incorporated into planetary bodies.
openaire   +2 more sources

Millimetre Observations of Maser-Emitting Planetary Nebulae

open access: yesGalaxies, 2022
Observations in the millimetre bands of maser-emitting planetary nebulae (PNe) are crucial to study their circumstellar molecular gas at the beginning of the PN phase.
Lucero Uscanga   +9 more
doaj   +1 more source

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