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heng xing de tong nian ( xia )
Author(s): 
Pages: 38-39
Year: Issue:  8
Journal: The Journal of UFO Research

Keyword:  主序星原始星星球恒星观测结果太阳质量对流不稳定收缩星际表面温度;
Abstract: <正>前主序星典型稠密核的质量一般都大于恒星的质量。因此,一定有某种机制可将多余质量扫走,并阻止质量不断由外面流入。大部分天文学家现在相信,在原始星球表面会喷出强烈的星际风,可以将流入的质量吹走,慢慢地驱散整个稠密核。星际风的想法并不是来自于理论的计算,由于广泛地观测到
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