Her X-1是中子星吗?

本文通过对Her X-1的X-ray观测结果和其他中子星X-ray时间变化特征和X-ray谱特征分析,对Her X-1是中子星提出质疑.并根据"电子-离子束缚态及其引发核过程"(简称:电子-离子束缚态)假说,时照太阳耀斑机制,认为Her X-1的辐射可能是它的伴星HZ-Her的耀斑.     

基于散体动力学理论的掘进机星轮装载机构研究

为了解决掘进机星轮对物料推力过大,物料因惯性而不随轮齿同步运动的问题,运用散体动力学理论分析掘进机装载机构的星轮轮齿推移物料的运动过程.建立力学和数学模型,推导出掘进机星轮机构装载过程中保持物料稳定运行的推力计算公式和轮齿许用加速度范围;并用计算机模拟轮齿推力与轮齿参数的关系,提出了轮齿推移物料的动力学模型和方程,为星轮装载机构的设计和研究提供了参考依据.     

图S_m∨S_n的均匀全色数

一个全染色满足||Ti|-|Tj||≤1时称为均匀的,其中|Ti|为染第i种颜色的元素数,所需最少染色数称为均匀全色数,记为χet(G)。文中得到了Sm∨Sn的均匀全色数。     

The amphibians and reptiles of Nosy Be (NW Madagascar) and nearby islands: a case study of diversity and conservation of an insular fauna

Surveys of the amphibians and reptiles on Nosy Be (an island off north-west Madagascar) and nearby islands were undertaken between 1991 and 2001 and are discussed here in view of biodiversity considerations and conservation efforts. Since Nosy Be is the type locality of several amphibian and reptile taxa, their exact status is of crucial importance for the nomenclatural stability of many groups of the Madagascan herpetofauna. A total of 20 amphibian and 61 reptile species (excluding marine reptiles) was confirmed for this archipelago. Other species (Mantidactylus horridus, Androngo elongatus, Typhlops madagascariensis, T. reuteri, Micropisthodon ochraceus and Pararhadinea melanogaster) were not found during these inventories, but are quoted in the literature or housed in herpetological collections, and are considered as likely to be present at Nosy Be. A further 18 taxa are tentatively excluded from its fauna, due to biogeographic incongruence and/or lack of reliable voucher specimens. Few taxa are so far only known from the island; they may represent endemics or may have been overlooked on the adjacent mainland. They are respectively Stumpffia pygmaea, Mabuya lavarambo, Lygodactylus h. heterurus, Lycodryas granuliceps and Typhlops reuteri. Heterixalus tricolor too is likely to be present on Nosy Be only, but the difference with respect to taxa present on the mainland needs to be confirmed. Several species are known from nearby islands and islets surveyed (11 amphibians and 26 reptiles). A few of them (Heterixalus 'variabilis', Kinixys belliana, Furcifer oustaleti, Mabuya comorensis, Paracontias milloti) are present on some of these islands but have not yet been found on Nosy Be. Much of the field research was conducted at Lokobe, a strict nature reserve still characterized by good forest coverage (typical of the Sambirano Domain), and an important area of biodiversity. With 15 amphibian and 45 reptile species, Lokobe hosts 81% of the overall Nosy Be herpetofauna: of the species found during our surveys, only Heterixalus tricolor, Hoplobatrachus tigerinus, Gehyra mutilata, Phelsuma dubia and Crocodylus niloticus were only found outside the reserve. In view of this, the protection of Lokobe should be assured and reinforced. Except for Lokobe, habitats on Nosy Be are largely anthropogenic, and have a lower species diversity, especially where there is intensive agriculture. At other sites (e.g. ylang-ylang and coffee plantations) and in forested bands along roads, species diversity is still high: careful management of these anthropogenic habitats might also assure the survivorship and conservation of a diverse herpetofauna outside the protected area.     

2—Banach空间中非扩张映象的不动点定理

本文在2-Banach空间中讨论非扩张映象不动点的存在性,得到了一些新的结果     

关于齿顶边星图的优美性

在齿轮图.的每个齿的齿顶分别加上 m_1,m_2,…,m_n,条悬挂边后构成的图称为齿顶边星图,记为,(m_1,m_2,…,m_n).本文给出了、(m_1,m_2…,m_n)的优美标号,从而证明了.(m_1,m_2,…,m_n)是优美图;当m_1=m_2=…,m_n=k 时,(k,k,…k)即为 k 顶边星图,于是解决了“所有的 k 顶边星图都是优美图”这一猜想.     

强磁场中的逆康普顿散射

本文根据非相对论情形(B/B_(cr)《1,hv/m_eC~2《1)强磁场中的康普顿散射微分截面,讨论了强磁场中低频光子与相对论电子的逆康普顿散射,并给出了呈幂律分布的低频光子与呈幂律分布的相对论电子相互作用产生的逆康顿散射谱,这可以用来解释γ射线爆高达几百KeV的低频倒转谱。     

用共振群方法计算~7Be的~3He-~4He集团态的E2、M1跃迁

该文假定~7Be的基态和第1,2,3激发态是~3He-~4He集团态,用共振群方法(RGM)计算这些态的本征能量和本征函数,并用这些函数计算了这些态之间的M1、E2跃迁几率,所得结果与实验基本符合,说明了~7Be的基态和第1,2,3激发态主要是~3He-~4He集团态,也说明了用RGM来研究核的集团态是很有效的,特别是理论计算的跃迁与实验的符合说明了计算中求得的各态的波函数是比较好的。     

汉代石氏星官研究

该文首次利用傅里叶分析法对《石氏星经》星表的观测年代进行了研究，认为星表观测年代为公元前７８年。并在此基础上复原了汉代的石氏星官，为进一步研究汉代星空提供了一个基础。     

关于双星系统的能量

本文利用广义相对论理论中的后牛顿近似结果，计算出双星系统的伴星的总能量．