The influence of feedback from massive stars on the formation and emergence of massive clusters

被引:0
作者
Dale, James E. [1 ,2 ]
机构
[1] Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany
[2] Excellence Cluster Universe, Boltzmannstr 2, D-85748 Garching, Germany
来源
FORMATION, EVOLUTION, AND SURVIVAL OF MASSIVE STAR CLUSTERS | 2017年 / 12卷 / S316期
关键词
stars: formation; galaxies: star clusters; ISM: kinematics and dynamics; H II REGIONS; RADIATIVE FEEDBACK; IONIZING FEEDBACK; STELLAR; FRAGMENTATION; ACCRETION; EVOLUTION; ENERGY; POPULATION; WINDS;
D O I
10.1017/S1743921315009734
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Massive star clusters are of fundamental importance both observationally, since they are visible at such great distances, and theoretically, because of their influence on the large-scale ISM. Understanding stellar feedback is a prerequisite for making sense of their formation and early evolution, since feedback influences cluster structure, star formation efficiency, and sets the timescales on which clusters emerge from their parent clouds to become optically visible. I review the progress made in understanding these issues from a numerical perspective.
引用
收藏
页码:177 / 183
页数:7
相关论文
共 63 条
[1]   The formation of the first star in the universe [J].
Abel, T ;
Bryan, GL ;
Norman, ML .
SCIENCE, 2002, 295 (5552) :93-98
[2]   Probing cluster formation under extreme conditions: massive star clusters in blue compact galaxies [J].
Adamo, A. ;
Ostlin, G. ;
Zackrisson, E. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2011, 417 (03) :1904-1912
[3]   Radiation-magnetohydrodynamic simulations of H II regions and their associated PDRs in turbulent molecular clouds [J].
Arthur, S. J. ;
Henney, W. J. ;
Mellema, G. ;
De Colle, F. ;
Vazquez-Semadeni, E. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2011, 414 (02) :1747-1768
[4]   The statistical properties of stars and their dependence on metallicity: the effects of opacity [J].
Bate, Matthew R. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2014, 442 (01) :285-313
[5]   Stellar, brown dwarf and multiple star properties from a radiation hydrodynamical simulation of star cluster formation [J].
Bate, Matthew R. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2012, 419 (04) :3115-3146
[6]   The importance of radiative feedback for the stellar initial mass function [J].
Bate, Matthew R. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2009, 392 (04) :1363-1380
[7]   The First Galaxies [J].
Bromm, Volker ;
Yoshida, Naoki .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 49, 2011, 49 :373-407
[8]   OUTFLOW-DRIVEN TURBULENCE IN MOLECULAR CLOUDS [J].
Carroll, Jonathan J. ;
Frank, Adam ;
Blackman, Eric G. ;
Cunningham, Andrew J. ;
Quillen, Alice C. .
ASTROPHYSICAL JOURNAL, 2009, 695 (02) :1376-1381
[9]   The first stellar cluster [J].
Clark, Paul C. ;
Glover, Simon C. O. ;
Klessen, Ralf S. .
ASTROPHYSICAL JOURNAL, 2008, 672 (02) :757-764
[10]   The Formation and Fragmentation of Disks Around Primordial Protostars [J].
Clark, Paul C. ;
Glover, Simon C. O. ;
Smith, Rowan J. ;
Greif, Thomas H. ;
Klessen, Ralf S. ;
Bromm, Volker .
SCIENCE, 2011, 331 (6020) :1040-1042