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You-Hua Chu & Robert A. Gruendl

Feedback from Massive YSOs and Massive Stars

(Volume 80 - Année 2011)
Article
Open Access

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.

Pour citer cet article

You-Hua Chu & Robert A. Gruendl, «Feedback from Massive YSOs and Massive Stars», Bulletin de la Société Royale des Sciences de Liège [En ligne], Volume 80 - Année 2011, 297 - 309 URL : https://popups.uliege.be/0037-9565/index.php?id=2768.

A propos de : You-Hua Chu

Astronomy Department, University of Illinois, Urbana, IL 61801, USA

A propos de : Robert A. Gruendl

Astronomy Department, University of Illinois, Urbana, IL 61801, USA