Results 1 to 10 of about 35,614 (300)
Accretion disks in luminous young stellar objects [PDF]
The Astronomy and Astrophysics Review, 2016 71 pages, 19 figures.
BELTRAN SOROLLA, MARIA TERESA +1 more
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Stellar Black Holes Can “Stretch” Supermassive Black Hole Accretion Disks
The Astrophysical Journal LettersStellar black holes (sBHs) are widely believed to exist in the accretion disks of active galactic nuclei (AGNs). Previous studies often focus on the transient emission produced by embedded sBHs. Here, we explore the possible observational consequences of
Shuying Zhou +5 more
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Stellar and Accretion Disk Parameters of the Close Binary HD 50526 [PDF]
The Astronomical Journal, 2021 Abstract We present a photometric and spectroscopic study of HD 50526, an ellipsoidal binary member of the group Double Periodic Variable stars. Performing data mining in photometric surveys and conducting new spectroscopic observations with several spectrographs during 2008–2015, we obtained orbital and stellar parameters of the system.
J. A. Rosales +7 more
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Disk Accretion and the Stellar Birthline [PDF]
The Astrophysical Journal, 1997 We present a simplified analysis of some effects of disk accretion on the early evolution of fully convective, low-mass pre-main-sequence stars. Our analysis builds on the previous seminal work of Stahler, but it differs in that the accretion of material occurs over a small area of the stellar surface, such as through a disk or magnetospheric accretion
Lee Hartmann +2 more
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How accretion of planet-forming disks influences stellar abundances
Astronomy & Astrophysics, 2023 Millimeter-sized dust grains experience radial velocities exceeding the gas velocities by orders of magnitude. The viscous evolution of the accretion disk adds disk material onto the central star’s convective envelope, influencing its elemental abundances, [X/H].
L.-A. Hühn, B. Bitsch
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Nonstationary magnetic microstructures in stellar thin accretion disks [PDF]
Physical Review E, 2013 14 text pages, 5 figures, to be published on ...
MONTANI, Giovanni, PETITTA, JACOPO
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Discovery of Two Different Full Disk Evolutionary Patterns of M-type T Tauri Stars with LAMOST DR8
The Astrophysical Journal, 2023 The full disk, full of gas and dust, determines the upper limit of planet masses, and its lifetime is critical for planet formation, especially for giant planets.
Hasitieer Haerken +4 more
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Tracing episodic accretion with NOEMA: FU Orionis-type stars and their millimeter environment [PDF]
EPJ Web of Conferences, 2022 The earliest phases of star formation are characterised by intense mass accretion from the circumstellar disk to the central star. One group of lowmass young stellar objects, FU Orionis-type stars (FUors) exhibit accretion rate peaks accompanied by ...
Fehér O. +6 more
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An Old, Metal-rich Accreted Stellar Component in the Milky Way Stellar Disk
The Astrophysical Journal, 2022 Abstract We study the possibility that the Milky Ways’ cool stellar disk includes mergers with ancient stars. Galaxies are understood to form in a hierarchical manner, where smaller (proto-)galaxies merge into larger ones. Stars in galaxies, like the Milky Way, contain in their motions and elemental abundance tracers of past events and ...
Diane K. Feuillet +3 more
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Outflows and particle acceleration in the accretion disks of young stars [PDF]
EPJ Web of Conferences, 2019 Magneto-gas-dynamic (MGD) outflows from the accretion disks of T Tauri stars with fossil large-scale magnetic fileld are investigated. We consider two mechanisms of the outflows: rise of the magnetic flux tubes (MFT) formed in the regions of efficient ...
Khaibrakhmanov Sergey, Dudorov Alexander
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