Artículo
Exploring Molecular Gas toward the Magellanic Bridge
Celis Peña, Mariela; Rubio, Mónica; Saldaño, Hugo Pablo
; Valdivia Mena, M. T.; Duvidovich, Laura Patricia
; Paron, Sergio Ariel
; Valdivia Mena, M. T.; Duvidovich, Laura Patricia
; Paron, Sergio Ariel
Fecha de publicación:
04/2024
Editorial:
IOP Publishing
Revista:
Research Notes of the AAS
e-ISSN:
2515-5172
Idioma:
Inglés
Tipo de recurso:
Artículo publicado
Clasificación temática:
Resumen
The Magellanic Bridge (MB) is a diffuse gas structure that connects the Large Magellanic Cloud with the Small Magellanic Cloud. The MB is the closest tidal interaction system between two galaxies to the Milky Way. Taking into account that young stellar objects are embedded in such gaseous structure, it is a unique laboratory to investigate gas dynamics and star formation processes in a very low metallicity environment. In this work we present a preview of the results obtained from observations made with the Atacama Pathfinder Experiment telescope toward some regions of the MB. Through the emission of the 12CO J = 2–1 line we characterize the molecular gas of these regions.
Palabras clave:
ISM: CLOUDS
,
ISM: MOLECULES
,
MAGELLANIC BRIDGE
,
GALAXY
Archivos asociados
Tamaño:
572.5Kb
Formato:
PDF
Licencia
Excepto donde se diga explícitamente, este item se publica bajo la siguiente descripción:
Creative Commons Attribution 2.5 Unported (CC BY 2.5)
Identificadores
Colecciones
Articulos(INENCO)
Articulos de INST.DE INVEST.EN ENERGIA NO CONVENCIONAL
Articulos de INST.DE INVEST.EN ENERGIA NO CONVENCIONAL
Citación
Celis Peña, Mariela ; Rubio, Mónica; Saldaño, Hugo Pablo; Valdivia Mena, M. T.; Duvidovich, Laura Patricia; et al.; Exploring Molecular Gas toward the Magellanic Bridge; IOP Publishing; Research Notes of the AAS; 8; 4; 4-2024; 1-4
Compartir
Altmétricas