Interaction of massive stars with their surroundings
Due to their short lifetimes but their enormous energy release in all stages of their lives massive stars are the major engines for the comic matter circuit. They affect not only their close environment but are also responsible to drive mass flows on galactic scales. Recent 2D models of radiation-driven and wind-blown HII regions are summarized which explore the impact of massive stars to the interstellar medium but find surprisingly small energy transfer efficiencies while an observable Carbon self-enrichment in the Wolf-Rayet phase is detected in the warm ionized gas. Finally,the focus is set on state-of-the-art modelling of HII regions and its present weaknesses with respect to uncertainties and simplifications but on a perspective of the requested art of their modelling in the 21st century.
Stars:supergiants (ISM:)HII regions ISM:kinematics and hydrodynamics galaxies:evolution
Gerhard Hensler
Institute of Astronomy,University of Vienna,Tuerkenschanzstr.17,1180 Vienna,Austria
国际会议
The 252th Symposium of the International Astronomical Union(国际天文学联合会第252届研讨会)
海南三亚
英文
309-316
2008-04-06（万方平台首次上网日期，不代表论文的发表时间）