Spin-down of Solar-mass Protostars in Magnetospheric Accretion Paradigm
Stellar spin is one of the fundamental quantities that characterize a star itself and its planetary system. Nevertheless, stellar spin-down mechanisms in protostellar and pre-main-sequence stellar phases have been a long-standing problem in star formation theory. To realize the spin-down, previous a...
Saved in:
Main Authors: | Shinsuke Takasao, Masanobu Kunitomo, Takeru K. Suzuki, Kazunari Iwasaki, Kengo Tomida |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/ada364 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Stellar Streams Reveal the Mass Loss of Globular Clusters
by: Yingtian Chen, et al.
Published: (2025-01-01) -
APOKASC-3: The Third Joint Spectroscopic and Asteroseismic Catalog for Evolved Stars in the Kepler Fields
by: Marc H. Pinsonneault, et al.
Published: (2025-01-01) -
Thermal Spectra of Warped and Broken Accretion Disks
by: J. Speicher, et al.
Published: (2025-01-01) -
Discovery of the Richest Pulsating Ultramassive White Dwarf
by: Francisco C. De Gerónimo, et al.
Published: (2025-01-01) -
Interactions of exoplanets with their environment
by: Strugarek, Antoine
Published: (2023-04-01)