Characterizing the 3D Kinematics of Young Stars in the Radcliffe Wave

We present an analysis of the kinematics of the Radcliffe Wave, a 2.7-kpc-long sinusoidal band of molecular clouds in the solar neighborhood recently detected via 3D dust mapping. With Gaia DR2 astrometry and spectroscopy, we analyze the 3D space velocities of \(\sim 1500\) young stars along the Rad...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	arXiv.org 2022-08
Hauptverfasser:	Tu, Alan J, Zucker, Catherine, Speagle, Joshua S, Beane, Angus, Goodman, Alyssa, Alves, João, Faherty, Jacqueline, Burkert, Andreas
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrometry Dust Kinematics Molecular clouds Physics - Astrophysics of Galaxies Radial velocity Solar neighborhood Stars Stellar oscillations
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!