Session II

نویسندگان

چکیده

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Session II

The striking histological similarity between ASH and NASH strongly suggests that they are due to similar pathogenic mechanisms. We have proposed the hypothesis that both are diseases of “two hits”. In this model the first hit is the development of steatosis and the second a trigger of necroinflammation, with the role of steatosis being to increase the liver’s sensitivity to the second hit. Cand...

متن کامل

Discussion: Session II

Background: The objective of this study was to systematically review randomized trials assessing therapeutic hypothermia as a treatment for term neonates with hypoxic ischemic encephalopathy. Methods: The Cochrane Central Register of Controlled Trials, MEDLINE, EMBASE, CINAHL databases, reference lists of identified studies, and proceedings of the Pediatric Academic Societies were searched in J...

متن کامل

Session II: Architectures

The Heidelberg High-Speed Transport System (HeiTS) is a new-generation end-to-end communication system currently under development at the IBM European Networking Center (ENC) in Heidelberg. HeiTS is aimed at a heterogeneous environment comprising several computers with different operating systems and a variety of underlying local, metropolitan, and wide-area networks. It incorporates both end-s...

متن کامل

Session 3 : Cancer II

s not provided. [14.30–14.50] Natural human IgG antibodies as tools for cancer therapy Stephanie Brandlein University of Wurzburg, Germany Abstracts not provided.s not provided. [14.50–15.10] Antibody-maytansinoid conjugates: A new generation of linkers to provide enhanced potency against target cancers Rajeeva Singh ImmunoGen, Inc., 830 Winter Street, Waltham, MA

متن کامل

Session II First Stars

How and when did the first generation of stars form at the end of the cosmic dark ages? Quite generically, within variants of the cold dark matter model of cosmological structure formation, the first sources of light are expected to form in ∼ 10M dark matter potential wells at redshifts z 20. I discuss the physical processes that govern the formation of the first stars. These so-called Populati...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Proceedings of the Royal Society of Medicine

سال: 1969

ISSN: 0035-9157

DOI: 10.1177/003591576906200934