HOW STARS INTERACT WITH THEIR LOCAL ENVIRONMENT IN CYGNUS-X


Por: Roman-Zuniga, C., Jimenez-Bailon, Elena, Zapata, Luis, Palau, Aina

Publicada: 1 ene 2017
Resumen:
We present some results on our investigations on the young stellar populations in the regions DR15 and DR21 in the Cygnus-X massive star formation complex. We provide some insight on processes associated with the presence or absence of massive stars, and the consequences this has on gas removal and early evolution of young clusters. Our use of multi wavelength data permits to define a clear picture of the recent history of the complexes and the interaction of the young stars with their local environment.

Filiaciones:
Roman-Zuniga, C.:
 Univ Nacl Autonoma Mexico, Inst Astron, Campus Ensenada,Km 103 Carr Tijuana, Ensenada 228601, Baja California, Mexico

Jimenez-Bailon, Elena:
 Univ Nacl Autonoma Mexico, Inst Astron, Campus Ensenada,Km 103 Carr Tijuana, Ensenada 228601, Baja California, Mexico

Zapata, Luis:
 UNAM, Inst Radioastron & Astrofis, Morelia, Michoacan, Mexico

Palau, Aina:
 UNAM, Inst Radioastron & Astrofis, Morelia, Michoacan, Mexico
ISSN: 14052059





REVISTA MEXICANA DE ASTRONOMIA Y ASTROFISICA, SERIE DE CONFERENCIAS
Editorial
Universidad Nacional Autonoma de Mexico, Patzcuaro, Michoacan, México
Tipo de documento: Proceedings Paper
Volumen: 49 Número:
Páginas: 109-109
WOS Id: 000411656000072