The molecular clump towards the eastern border of SNR G18.8+0.3
Aims. The eastern border of the SNR G18.8+0.3, close to an HII regions complex, is a very interesting region for studying the molecular gas that it is probably in contact with the supernova remnant (SNR) shock front. Methods. We observed this region using the Atacama Submillimeter Telescope Experime...
Guardado en:
Publicado: |
2012
|
---|---|
Materias: | |
Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v547_n_p_Paron http://hdl.handle.net/20.500.12110/paper_00046361_v547_n_p_Paron |
Aporte de: |
Ejemplares similares
-
The molecular clump towards the eastern border of SNR G18.8+0.3
por: Paron, S., et al. -
The southern molecular environment of SNR G18.8+0.3
Publicado: (2015) -
The southern molecular environment of SNR G18.8+0.3
por: Paron, S., et al. -
Study of the molecular clump associated with the high-energy source HESS J1858+020
Publicado: (2011) -
Study of the molecular clump associated with the high-energy source HESS J1858+020
por: Paron, S., et al.