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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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Detalles Bibliográficos
Autores principales:	Pérez-Couto, Xabier, Torres, Santiago, Miret-Roig, Nuria, Anders, Friedrich, Mustill, Alexander J., Villaver, Eva, Manteiga, Minia
Formato:	Preprint
Publicado:	2026
Materias:	Astrophysics of Galaxies Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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