柴达木盆地东北缘中中新世以来古气候变化

全球变冷、青藏高原隆升以及特提斯洋海退被认为是控制亚洲大陆新生代气候变化的三大因素,然而由于长时间尺度古气候记录的匮乏,对于三者影响的认识并不清晰。柴达木盆地是青藏高原北部最大的一个封闭盆地,发育巨厚且连续的新生代地层,详细记录了周缘山体构造隆升过程和区域气候演化历史。本文通过柴达木盆地东北缘怀头他拉剖面的中中新世-早更新世沉积物气候代用指标碳酸盐、硫酸根和氯离子含量分析,显示该研究区中中新世以来气候变化经历了15.3~13.0Ma相对湿润、13.0~6.6Ma半干旱-半湿润和6.6~1.8Ma干旱的3个演化阶段。结合生物特征和前人研究成果,认为柴达木盆地干旱化历史可能从中中新世13Ma左右开始逐步发展,而真正意义上的干旱化始于6.6Ma以来。全球变冷是控制柴达木盆地干旱气候形成和发展的主导因素,同时青藏高原晚期持续阶段性的强烈隆升起到了催化剂的作用。     

恒星的主序后演化

本文按质量把恒星分为四类:一、小质量恒星0.07M_☉相似文献   

HD 104237,εCha和HD 100546的演化状态

根据Ｈｉｐｐａｒｃｏｓ的资料和ＴＤ－１对εＣｈａ和ＨＤ１００５４６的紫外观测资料讨论了εＣｈａ、ＨＤ１０４２３７和ＨＤ１００５４６在赫罗图上的位置以及它们的演化状态．     

The Effect of Central Baryonic Cores in Dark Halos on the Evaluation of Strong Lensing Probabilities

We present an estimate of the strong lensing probability by dark halos, with emphasis on the role of the baryonic matter arising purely from radiative cooling. We treat the contribution of the cooled baryons optimistically with all the cooled baryons confined within a central core, and including no feedback process from stellar evolution. Our two-component model provides a strong lensing probability that is in good agreement with the observed distribution of multiple images of quasars, provided that the cooled baryons are deposited within a spherical region of radius of 0.1 times the virial radius and follow an isothermal profile. It is pointed out that strong lensing may be used as an additional probe‘of baryon physics in dark halos though this may meanwhile complicate the test of the inner density profiles of dark matter in halos using the observed strong lensing probability.     

A Note on the Mixing Length Theory and Massive Star Evolution

1 INTRODUCTIONThe mixing length theory (MLT) for stellar convection originally developed by Vitense(1953, 1958) has been the most popularly used local convection theory in the studies of stellarstructure and evolution. The theory was later modified and revised by many investigators,who suggested some different expressions. In fact, MLT is not a real hydrodynamic theory,rather, it is a simple "ballistic" theory which traces the motion of imaginary convective elements. In reality j stell…     

恒星内部电荷屏幕对电子俘获反应的影响

本文分析了在恒星环境下，电荷强屏蔽对原子核电子俘获反应的影响，分析中忽略了电荷屏幕对核跃迁矩阵元的影响。作为例子，分别讨论了电荷屏蔽对核素＾３３Ｓ、＾３０Ｐ和＾５７Ｆｅ的电子俘获率的影响。结果表明：在较低温度和较高密度下，由于电荷屏蔽，其电子俘获率相对于无屏蔽情形有明显降低，这可能对恒星晚期演化和超新星爆发理论带来明显的影响。     

星系演化探测器GALEX

空间天文学发展了几十年,在近、远紫外波段,虽然各式各样的卫星有很多,但过去的科学实践更强调获得天体的紫外光谱,尤其是银河系中恒星的光谱。而拍摄天体紫外图像的卫星,