The HII region G35.673-00.847: Another case of triggered star formation?

Aims. As part of a systematic study that we are performing to increase the observational evidence of triggered star formation in the surroundings of HII regions, we analyze the ISM around the HII region G35.673-00.847, a poorly studied source. Methods. Using data from the large-scale surveys Two Mic...

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Detalles Bibliográficos
Publicado:	2010
Materias:	HII regions ISM: clouds stars: formation All-sky survey Galactic plane surveys Gravitational instability H II regions ISM : clouds Mid-IR emissions Molecular gas Molecular shells Multi-wavelength study Semi-ring Star formations Surrounding materials Systematic study Clouds Stars Surveys
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v525_n8_p_Paron http://hdl.handle.net/20.500.12110/paper_00046361_v525_n8_p_Paron
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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