Bulletin de la Société Royale des Sciences de Liège

0037-9565 1783-5720

 

sinds 05 februari 2011 :
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E. R. Parkin, J. M. Pittard, M. G. Hoare, N. J. Wright & J. J. Drake

The interactions of winds from massive young stellar objects

(Volume 80 - Année 2011)
Article
Open Access

Abstract

The supersonic stellar and disk winds possessed by massive young stellar objects will produce shocks when they collide against the interior of a pre-existing bipolar cavity (resulting from an earlier phase of jet activity). The shock heated gas emits thermal X-rays which may be observable by spaceborne observatories such as the Chandra X-ray Observatory. Hydrodynamical models are used to explore the wind-cavity interaction. Radiative transfer calculations are performed on the simulation output to produce synthetic X-ray observations, allowing constraints to be placed on model parameters through comparisons with observations. The model reveals an intricate interplay between the inflowing and outflowing material and is successful in reproducing the observed X-ray count rates from massive young stellar objects.

Om dit artikel te citeren:

E. R. Parkin, J. M. Pittard, M. G. Hoare, N. J. Wright & J. J. Drake, «The interactions of winds from massive young stellar objects», Bulletin de la Société Royale des Sciences de Liège [En ligne], Volume 80 - Année 2011, 246 - 250 URL : http://bibli-cloud15.segi.ulg.ac.be/0037-9565/index.php?id=2719.

Over : E. R. Parkin

Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium, and School of Physics and Astronomy, The University of Leeds, UK

Over : J. M. Pittard

School of Physics and Astronomy, The University of Leeds, UK

Over : M. G. Hoare

School of Physics and Astronomy, The University of Leeds, UK

Over : N. J. Wright

Harvard-Smithsonian Center for Astrophysics, USA

Over : J. J. Drake

Harvard-Smithsonian Center for Astrophysics, USA