A view of Large Magellanic Cloud HII regions N159, N132, and N166 through the 345-GHz window

We present results obtained towards the HII regions N159, N166, and N132 from the emission of several molecular lines in the 345 GHz window. Using Atacama Submillimetre Telescope Experiment, we mapped a 2.4 arcmin × 2.4 arcmin region towards the molecular cloud N159- W in the 13CO J = 3-2 line and o...

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Detalles Bibliográficos
Autores principales: Paron, S., Ortega, M.E., Fariña, C., Cunningham, M., Jones, P.A., Rubio, M.
Formato: JOUR
Materias:
Galaxies
HII regions
ISM
ISM-Magellanic Clouds
Molecules
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00358711_v455_n1_p518_Paron
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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