Study of the molecular and ionized gas in a possible precursor of an ultra-compact H II region
Aims. We aim to study the molecular and the ionized gas in a possible precursor of an ultra-compact H ii region to contribute to the understanding of how high-mass stars build-up their masses once they have reached the zero-age main sequence. Methods. We carried out molecular observations toward the...
Guardado en:
| Autores principales: | Ortega, M.E., Paron, S., Giacani, E., Celis Peña, M., Rubio, M., Petriella, A. |
|---|---|
| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00046361_v606_n_p_Ortega |
| Aporte de: |
Ejemplares similares
-
Study of the molecular and ionized gas in a possible precursor of an ultra-compact H II region
Publicado: (2017) -
Near-IR imaging toward a puzzling young stellar object precessing jet
por: Paron, S., et al. -
Near-IR imaging toward a puzzling young stellar object precessing jet
Publicado: (2016) -
The molecular gas around the luminous blue variable star G24.73+0.69
por: Petriella, A., et al. -
A molecular outflow revealing star formation activity in the vicinity of the HII region G034.8-0.7 and the SNR W44
por: Paron, S., et al.