Results 101 to 110 of about 206 (176)

Unveiling the Dual Nature of V1180 Cas: UXor-like Dips and EXor-like Bursts across a Decade

open access: yesThe Astrophysical Journal
We present a detailed analysis of the long-term photometric and spectroscopic evolution of V1180 Cas over a decade, aiming to identify the dominant mechanisms behind its variability. We combine multiband light curves from 1999 to 2025 with over 30 epochs
Tarak Chand   +17 more
doaj   +1 more source

The accretion process on protostars

open access: yesFrontiers in Astronomy and Space Sciences
The process of mass accretion onto Young Stellar Objects (YSOs) plays a fundamental role in determining the final stellar mass and setting the initial conditions for planet formation.
Eleonora Fiorellino   +2 more
doaj   +1 more source

A Multiwavelength, Multiepoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. III. Optical Spectra

open access: yesThe Astrophysical Journal
Classical T Tauri Stars (CTTSs) are highly variable stars that possess gas- and dust-rich disks from which planets form. Much of their variability is driven by mass accretion from the surrounding disk, a process that is still not entirely understood.
John Wendeborn   +22 more
doaj   +1 more source

Magnetic reconnection in partially ionized plasmas. [PDF]

open access: yesProc Math Phys Eng Sci, 2020
Ni L, Ji H, Murphy NA, Jara-Almonte J.
europepmc   +1 more source

The Pre-outburst Properties of the FU Ori Object HBC 722

open access: yesThe Astrophysical Journal Letters
FU Ori outbursts are thought to play an important role in stellar assembly and the evolution of protoplanetary disks. However, the progenitor young stellar objects are largely uncharacterized.
Gregory J. Herczeg, Bo Reipurth
doaj   +1 more source

A Multiwavelength, Multiepoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. I. HST Far-UV and Near-UV Spectra

open access: yesThe Astrophysical Journal
The classical T Tauri star (CTTS) stage is a critical phase of the star and planet formation process. In an effort to better understand the mass accretion processes, which can dictate future stellar evolution and planet formation, a multiepoch ...
John Wendeborn   +19 more
doaj   +1 more source

LAMOST Young Stellar Objects. I. Spectroscopically Identifying and Characterizing M-type YSOs

open access: yesThe Astrophysical Journal
This study utilized Large sky Area Multi-Object fiber Spectroscopic Telescope (LAMOST) low-resolution spectra to identify M-type young stellar objects (YSOs) and characterize their accretion signatures.
Xiang-Song Fang   +3 more
doaj   +1 more source

Revisiting the case of R Monocerotis: Is CO removed at R < 20 au?<sup>⋆</sup>. [PDF]

open access: yesAstron Astrophys, 2018
Alonso-Albi T   +6 more
europepmc   +1 more source

The Turbulent Dynamo. [PDF]

open access: yesJ Fluid Mech, 2021
Tobias SM.
europepmc   +1 more source

Binarity and Accretion in AGB Stars: HST/STIS Observations of UV Flickering in Y Gem. [PDF]

open access: yesAstrophys J, 2018
Sahai R   +5 more
europepmc   +1 more source

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