The interstellar medium and the massive stellar content towards the SNR G18.1-0.1 and neighbouring Hii regions

We perform a multiwavelength study of the SNR G18.1-0.1 and nearby several HII regions (infrared dust bubbles N21 and N22, and the HII regions G018.149-00.283 and G18.197-00.181). Our goal is to provide observational evidence supporting the view that massive stars are usually born in clusters from t...

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Autores principales: Paron, S., Weidmann, W., Ortega, M.E., Colombo, J.F.A., Pichel, A.
Formato: JOUR
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00358711_v433_n2_p1619_Paron
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