Titlebook: Jets in Young Stellar Objects; Theory and Observati A. J. L. Fernandes,P. J. V. Garcia,J. J. G. Lima Book 2003 Springer Science+Business Me

PON

Daniel F.M. Folhanducting experiments, it is important to be mindful of what scale to sample at; the “correct” scale depends on the research question and the organism(s) of interest. Frequently, patterns seen at one scale will be different – even opposite – at another scale, which introduces difficulties with extrap

排名真古怪

Suzan Edwardst tools and techniques than what researchers working in terrestrial landscapes use. I illustrate how landscape ecologists can learn from collaborations with marine biologists, aquatic, behavioural and acoustic ecologists to develop experimental approaches that address questions about space use in th

雪白

largesse

http://image.papertrans.cn/j/image/500886.jpg

Digitalis

Star-Driven Wind and Jet Models-wind models. We emphazise the roles of the magnetic rotator and the disk in the formation and the evolution of the jet. We conjecture that with time both the efficiency of the magnetic rotator and the role of the disk as a primary source for the wind decline.

強(qiáng)制性

Continuum Excess Emission in Young Low Mass Stars understanding about the CTTS systems impinges directly on our ability to achieve a deeper knowledge of the final stages of low mass stars formation, of the pre-main sequence history of the Sun and even on the processes that lead to planet formation. Here I present a portion of the . of the CTTS systems and some . in this field.

歡呼

Coronary-Spasm

跳動(dòng)

altruism

A.I. GóMez De Castro,C. Ferro-FontáNst for the audience, in which interpretation and meaning are forever suspended in the act of revision; a play in which the question of what and who has been represented is elusive. Instead of giving his audience a ‘retrospect’ of his life, Krapp is forever ‘embarking’ on a new retrospect. It is, per