The structure and kinematics of the ISM around HD 192281

Aims. This work aims at investigating the interaction of HD 192281 (O5 Vn((f))p) with its local ISM. The purpose is to analyse the effects that a massive star has on the structure and kinematics of its surrounding gas. Methods. To carry out this study, we used high-resolution radio continuum and 21-...

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Detalles Bibliográficos
Publicado: 2011
Materias:
ISM: bubbles
ISM: structure
outflows
Stars: individual: HD 192281
Stars: mass-loss
Stars: winds
Kinematics
Plasma shock waves
Surveys
Stars
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v532_n_p_Arnal
http://hdl.handle.net/20.500.12110/paper_00046361_v532_n_p_Arnal
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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