描述了通过路易斯酸催化的(a)三甲基硅烷化的6-烷基-4-烷基硫尿嘧啶与1-O-乙酰基-2,3,5-三-O-苯甲酰基-β-的缩合反应合成6-烷基尿苷的立体选择程序。 D-核呋喃糖(ABR)和(b)三甲基甲硅烷基化的6-烷基-3-苄基尿嘧啶与ABR。随后通过使用配合物BBr3-THF的新的改性方法,使用1N三氟乙酸除去4-甲硫基,并除去3-苄基。此外,通过依次用SeO 2氧化并用四丁基硼氢化铵还原6-甲基尿苷(5)获得6-(羟甲基)尿苷(39)和5-氟-6-(羟甲基)尿苷(40)。分别通过39和40的DAST处理,获得了5-氟-6-甲基尿苷和3-氟-6-甲基尿苷(35),以及它们相应的6-氟甲基同源物41和42。对于前述关于糖基键的固定顺式构象的所有核苷,1 H NMR光谱进一步证实戊糖环主要存在于构象N(3'-内)。大多数核苷是大肠杆菌嘧啶核苷磷酸化酶的弱底物。其中两个39和41具有6-C
Promotional effect of ionic liquids in electrophilic fluorination of methylated uracils
作者:Gennady I. Borodkin、Innokenty R. Elanov、Yury V. Gatilov、Vyacheslav G. Shubin
DOI:10.1039/c6ra10850d
日期:——
A novel efficient protocol has been developed for fluorination of methylated uracils involving a stoichiometric amount of ionicliquid (IL) in alcohols. The fluorination of 6-methyluracil and 1,3,6-trimethyluracil has been carried out using the electrophilic fluorinating reagent Selectfluor™ (F-TEDA-BF4) in MeOH and EtOH solvents with the formation of 5-fluoro-6-methyluracil, 5-fluoro-1,3,6-trimethyluracil
Process for fluorinating uracil and derivatives thereof
申请人:PCR, Inc.
公开号:US03954758A1
公开(公告)日:1976-05-04
Direct fluorination of uracil and its derivatives, in the presence of an aqueous solvent, by fluorine gas to produce 5-fluorouracil and 5-fluorouracil derivatives is disclosed. Novel compounds produced by the reaction, such as 5,5-difluoro-6-hydroxy-5,6-dihydrouracil are also disclosed. The derivatives of 5-fluorouracil are useful as germicidal agents while 5-fluorouracil itself is a known cancer chemotherapy agent.
Direct fluorination of uracil and its derivatives, in the presence of an aqueous solvent, by fluorine gas to produce 5-fluorouracil and 5-fluorouracil derivatives is disclosed. Novel compounds produced by the reaction, such as 5,5-difluoro-6-hydroxy-5,6-dihydrouracil are also disclosed. The derivatives of 5-fluorouracil are useful as germicidal agents while 5-fluorouracil itself is a known cancer chemotherapy agent.
Source regions and timescales for the delivery of water to the Earth
作者:A. Morbidelli、J. Chambers、J. I. Lunine、J. M. Petit、F. Robert、G. B. Valsecchi、K. E. Cyr
DOI:10.1111/j.1945-5100.2000.tb01518.x
日期:2000.11
Abstract—In the primordial solar system, the most plausible sources of the water accreted by the Earth were in the outer asteroid belt, in the giant planet regions, and in the Kuiper Belt. We investigate the implications on the origin of Earth's water of dynamical models of primordial evolution of solar system bodies and check them with respect to chemical constraints. We find that it is plausible that the Earth accreted water all along its formation, from the early phases when the solar nebula was still present to the late stages of gas‐free sweepup of scattered planetesimals. Asteroids and the comets from the Jupiter‐Saturn region were the first water deliverers, when the Earth was less than half its present mass. The bulk of the water presently on Earth was carried by a few planetary embryos, originally formed in the outer asteroid belt and accreted by the Earth at the final stage of its formation. Finally, a late veneer, accounting for at most 10% of the present water mass, occurred due to comets from the Uranus‐Neptune region and from the Kuiper Belt. The net result of accretion from these several reservoirs is that the water on Earth had essentially the D/H ratio typical of the water condensed in the outer asteroid belt. This is in agreement with the observation that the D/H ratio in the oceans is very close to the mean value of the D/H ratio of the water inclusions in carbonaceous chondrites.