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| DOI | 10.1051/0004-6361/201014369 | ||||
| Año | 2011 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Conclusions. We discuss the possible connections between the molecular gas at the CND and the GMCs using the HNCO/SiO, SiO/CS, and HNCO/CS intensity ratios as probes of distance to the Central cluster. In particular, the HNCO/SiO intensity ratio is proved to be an excellent tool for evaluating the distance to the center of the different gas components.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Amo-Baladron, M. A. | - |
CSIC INTA - España
Centro de Astrobiología (CSIC-INTA) - España |
| 2 | Martín-Pintado, J. | Hombre |
CSIC INTA - España
Centro de Astrobiología (CSIC-INTA) - España |
| 3 | Martin, S. | - |
ESO - Chile
Harvard Smithsonian Ctr Astrophys - Estados Unidos |
| Agradecimiento |
|---|
| The authors would like to thank Prof. M. Tsuboi and D. M. Montero-Castano for kindly providing their CS(1-0) and HCN(4-3) data, respectively. We also thank the referee for the suggestions. This work was supported by the Spanish Ministerio de Ciencia e Innovacion under project ESP2007-65812-C02-01. |