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A homogeneous three-dimensional view of Molecular Cloud kinematics out to 2.5 kpc. Using Young Stellar Objects and Open Clusters as complementary tracers

Fuente: arXiv

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Détails bibliographiques
Auteurs principaux:	Pérez-Couto, Xabier, Torres, Santiago, Miret-Roig, Nuria, Anders, Friedrich, Mustill, Alexander J., Villaver, Eva, Manteiga, Minia
Format:	Preprint
Publié:	2026
Sujets:	Astrophysics of Galaxies Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

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