- Portada
- Volume 80 - Année 2011
- Feedback from Massive YSOs and Massive Stars
Vista(s): 342 (7 ULiège)
Descargar(s): 613 (9 ULiège)
Feedback from Massive YSOs and Massive Stars
![Open Access](images/Open_Access.png)
Documento adjunto(s)
Anexidades
Abstract
Massive stars are powerful sources of radiation, stellar winds, and supernova explosions. The radiative and mechanical energies injected by massive stars into the interstellar medium (ISM) profoundly alter the structure and evolution of the ISM, which subsequently influences the star formation and chemical evolution of the host galaxy. In this review, we will use the Large Magellanic Cloud (LMC) as a laboratory to showcase effects of energy feedback from massive young stellar objects (YSOs) and mature stars. We will also use the Carina Nebula in the Galaxy to illustrate a multi-wavelength study of feedback from massive star.
Para citar este artículo
Acerca de: You-Hua Chu
Astronomy Department, University of Illinois, Urbana, IL 61801, USA
Acerca de: Robert A. Gruendl
Astronomy Department, University of Illinois, Urbana, IL 61801, USA