Molecules at high redshift: The evolution of the cool phase of protogalactic disks

被引:51
作者
Norman, CA [1 ]
Spaans, M [1 ]
机构
[1] SPACE TELESCOPE SCI INST, BALTIMORE, MD 21218 USA
关键词
early universe; galaxies; formation; molecular processes; stars;
D O I
10.1086/303940
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the formation of molecular hydrogen, after The epoch of reionization, in the context of canonical galaxy formation theory due to hierarchical clustering. There is an initial epoch of H-2 production in the gas phase through the H- route that ends at a redshift of order unity. We assume that the fundamental units in the gas phase of protogalaxies during this epoch are similar to diffuse clouds found in our own Galaxy, and we restrict our attention to protogalactic disks, although some of our analysis applies to multiphase halo gas. Giant molecular clouds are not formed until lower redshifts. Star formation in the protogalactic disks can become self-regulated. The process responsible for the feedback is the heating of the gas by the internal stellar radiation field that can dominate the background radiation field at various epochs. If the gas is heated to above 2000-3000 K, the hydrogen molecules are collisionally dissociated, and we assume that in their absence the star formation process is strongly suppressed because of insufficient cooling. As we demonstrate by the analysis of phase diagrams, the H-2-induced cool phase disappears. A priori, the cool phase with molecular hydrogen cooling can only achieve temperatures greater than or equal to 300 K. Consequently, it is possible to define a maximum star formation rate during this epoch. Plausible estimates give a rate of less than or similar to 0.2-2 M. yr(-1) for condensations corresponding to 1 sigma and 2 sigma initial density fluctuations. For more massive structures, this limit is relaxed and in agreement with observations of high-redshift galaxies. Therefore, the production of metals and dust proceeds slowly in this phase. This moderate epoch is terminated by a phase transition to a cold, dense, and warm neutral/ionized medium once the metals and dust have increased to a level Z approximate to 0.03-0.1 Z.. Then (1) atoms and molecules such as C, O, and CO become abundant and cool the gas to below 300 K; (2) the dust abundance has become sufficiently high to allow shielding of the molecular gas; and (3) molecular hydrogen formation can occur rapidly on grain surfaces. This phase transition occurs at a redshift of approximately 1.5, with a fiducial range of 1.2 less than or equal to z less than or equal to 2, and initiates the rapid formation of molecular species, giant molecular clouds, and stars. Consequently, the delayed initiation of the cold phase in the interstellar medium of protostellar disks at a metallicity of Z less than or similar to 0.1 Z. is a plausible physical reason why the formation phase of the stellar disks of the bulk of the galaxies occurs only at a redshift of order unity. The combination of feedback and a phase transition provides a natural resolution of the G-dwarf problem.
引用
收藏
页码:145 / 154
页数:10
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