HIGH-MASS STAR FORMATION

被引：11

作者：

Schilke, P. ^{[1
]}

机构：

[1] Univ Cologne, Inst Phys 1, Zulpicher Str 77, D-50937 Cologne, Germany

来源：

6TH ZERMATT ISM-SYMPOSIUM: CONDITIONS AND IMPACT OF STAR FORMATION: FROM LAB TO SPACE: IN MEMORY OF CHARLES H. TOWNES | 2016年 / 75-76卷

关键词：

MOLECULAR CLOUDS; RADIATIVE FEEDBACK; ROTATING TOROIDS; CYGNUS-X; ACCRETION; DISK; CORES; PROTOSTARS; COLLAPSE; ALMA;

D O I：

10.1051/eas/1575046

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A review on current theories and observations of high-mass star formation is given. Particularly the influence of magnetic fields and feedback mechanisms, and of varying initial conditions on theories are discussed. The, in my biased view, most important observations to put strong constraints on models of high-mass star formation are presented, in particular bearing on the existence and properties of high mass starless cores, the role of filaments in the mass transport to high mass cores, and the properties of disks around high-mass stars.

引用

页码：227 / 235

页数：9

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