THE ROLE OF THERMAL INSTABILITIES ON THE THEORETICAL MASS FUNCTION OF MACHOs

E. M. DE GOUVEIA DAL PINO; J. E. HORVATH; J. A. DE FREITAS PACHECO

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THE ROLE OF THERMAL INSTABILITIES ON THE THEORETICAL MASS FUNCTION OF MACHOs

机译：热不稳定性在宏观理论质量函数中的作用

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We analyze the primordial protogalactic gas to investigate the role of thermal instabilities in the formation of condensations that could contribute to the MACHO mass function. We find that the previrialized protogalaxy could have undergone a thermally unstable regime, which defines a peak in mass condensations starting around 0.1 solar mass after being reprocessed by the environment that may be identified as giving origin to the MACHOs. Effects of magnetic fields on this instability-driven MACHOs scenario are also addressed.

机译：我们分析原始原银河气体，以调查热不稳定性在缩合形成中的作用，该缩合可能有助于MACHO质量功能。我们发现，经过预病毒化的原星系可能经历了热不稳定的过程，该过程在经过可能被认为是MACHOs起源的环境后处理之后，在0.1太阳质量附近定义了质量凝结的峰值。还讨论了磁场对这种不稳定驱动的MACHOs情况的影响。

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来源
《The Astrophysical journal》 |1996年第2pt2期|p.L97-L100|共4页
作者
E. M. DE GOUVEIA DAL PINO; J. E. HORVATH; J. A. DE FREITAS PACHECO;
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作者单位

Instituto Astronomico e Geofisico, Universidade de Sao Paulo, Avenida Miguel Stefano 4200 (04301-904), Sao Paulo-SP, Brazil;

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正文语种 eng
中图分类天文学;
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THE ROLE OF THERMAL INSTABILITIES ON THE THEORETICAL MASS FUNCTION OF MACHOs

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