986 resultados para B-7


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C13H12F3NO2, M(r) = 271.2, triclinic, P1BAR, a = 5.029 (2), b = 7.479 (2), c = 17.073 (5) angstrom, alpha = 97.98 (2), beta = 95.54 (3), gamma = 103.62 (3)-degrees, V = 612.4 (4) angstrom 3, Z = 2, D(m) = 1.463, D(x) = 1.471 g cm-3, lambda(Mo K-alpha) = 0.71069 angstrom, mu = 1.23 cm-1, F(000) = 280, T = 298 K, final R value is 0.041 for 2047 observed reflections with \F(omicron)\ greater-than-or-equal-to 6-sigma(\F(omicron)\). The N-C(sp2) bond length is 1.356 (2) angstrom. The N and C atoms of the ethylamino group deviate by < 0.15 angstrom from the plane of the aromatic ring. Short intramolecular contacts, C(3)...F(17) 2.668 (3) angstrom [H(3)...F(17) 2.39 (2) angstrom, C(3)-H(C3)...F(17) 98 (1)-degrees], C(5)...F(18) 3.074 (3) and C(5)...F(19) 3.077 (3) angstrom exist in the structure. The crystal structure is stabilized by intermolecular N-H...O hydrogen bonds with N(12)-H(N12) 0.79 (3), H(N12)...O(11)' 2.36 (3), N(12)...O(11)' (x - 1, y + 1, z) 3.105 (3) angstrom and N(12)-H(N12)...O(11)' 155 (2)-degrees.

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人类活动产生的氯氟烃化合物破坏了大气臭氧层,导致了到达地球表面的UV-B辐射大幅度增加。UV-B辐射增强可以影响到植物的生长、形态与发育等各个方面,因此有关增强UV-B辐射对植物的影响,及其与许多环境因子复合作用的研究都已经广泛开展。但是增强UV-B辐射与温度,特别是与低温的相互作用的研究报道很少。在北半球的晚秋至早春这段时期里,一些越冬生长的植物将面临着UV-B辐射增强和低温的双重胁迫,因此,迫切需要进行UV-B辐射和低温生长环境下植物的响应及其机制的研究。 以人工气候生长室中生长的冬小麦(Triticum aestivum)幼苗为试验材料,研究了低剂量(4.2 kJ m-2 d-1 UV-BBE,LUVB)和较高剂量(7.0 kJ m-2 d-1 UV-BBE,HUVB)UV-B辐射处理对20/16℃条件下幼苗抗寒力的交叉适应性及其抗氧化系统的反应;同时还研究了在两种生长温度(25/20℃和10/5℃)条件下,低剂量(4.2 kJ m-2 d-1 UV-BBE,LUVB)和超高剂量(10.3 kJ m-2 d-1 UV-BBE,SHUVB)UV-B辐射处理幼苗的生长速率、光合与荧光参数、叶黄素循环色素、抗氧化系统、以及抗寒性和酚类物质等生理反应,以期阐明不同温度条件下生长的冬小麦对UV-B辐射的生长、光合作用以及抗寒性响应与适应机制。主要结果如下: 1.在LUVB辐射处理下,在20/16℃和25/20℃条件下生长的冬小麦幼苗LT50值都显著降低,HUVB辐射处理对在20/16℃条件下生长的幼苗LT50值也可以显著降低,而SHUVB辐射对25/20℃条件下生长的幼苗LT50值没有显著影响。但是,LUVB和SHUVB辐射处理都导致了10/5℃条件下生长的幼苗LT50值的显著增加。表明适当的UV-B辐射能增强较高温度(20/16℃或25/20℃)条件下冬小麦幼苗的抗寒力,即表现出对冷冻低温的交叉适应性,但低温(10/5℃)生长条件却削弱了UV-B辐射下冬小麦的抗寒能力。 2.在20/16℃条件下接受UV-B辐射预处理的幼苗在-6℃条件下冷冻胁迫6 h再缓慢恢复6 h后,与未进行UV-B辐射处理的对照相比,其叶片过氧化氢酶(CAT)、愈创木酚过氧化物酶(GPX)、谷胱甘肽还原酶(GR)活性,谷胱甘肽氧化还原比例(GSH/GSSG)都显著提高,而由硫代巴比妥酸反应物质(TBARS)代表的膜质过氧化程度显著低于对照。此外,UV-B辐射期间处理幼苗的H2O2含量较对照显著增加,而冷冻恢复以后却明显低于对照。表明UV-B辐射诱导的抗寒力的提高应该与冷冻恢复后植株体内抗氧化系统的上调表达有关,H2O2可能参与了UV-B辐射对低温的交叉适应的信号传导。 3.除25/20℃生长条件下的LUVB处理的小麦幼苗外,UV-B辐射显著降低幼苗的相对生长速率(RGR)、净光合速率(Pn)、光系统II最大量子产量(Fv/Fm)、光系统II实际量子产量((F΄m−Fs)/F΄m)以及光化学淬灭(qP),但是UV-B辐射并不影响叶片胞间CO2浓度(Ci),而且冬小麦幼苗生长和光合作用的抑制被增加的UV-B辐射剂量和降低的温度加强。UV-B辐射引起的光抑制由非气孔限制所导致,而且主要与PS II光化学效率降低有关。 4.UV-B辐射显著增加了两个温度条件(20/16℃或25/20℃)下生长的冬小麦幼苗叶黄素循环过程中紫黄素(V)的合成,但抑制了V向玉米黄质(Z)的转化,从而造成了对照与LUVB辐射处理幼苗之间的叶片中脱环氧化比例(DEPS)和NPQ无显著性差异,但SHUVB辐射处理幼苗叶片中DEPS和NPQ显著降低。因此,在本试验条件下,增强UV-B辐射处理的冬小麦可能并不通过热耗散形式形成光保护机制,光抑制形成的过剩激发能的耗散可能更多地通过代谢途径来实现。 5.UV-B辐射处理提高了在25/20℃条件下幼苗的超氧化物歧化酶(SOD)、抗坏血酸过氧化物酶(APX)和GR等活性,以及抗坏血酸氧化还原比例(AsA/DHA)和GSH/GSSG;但是在10/5℃下,UV-B辐射除了导致SOD和CAT活性升高之外,对APX活性和AsA/DHA并不产生明显影响,但GPX和GSH/GSSG则显著降低。说明UV-B辐射幼苗的抗氧化系统在较高生长温度下显著地增强,而在低温10/5℃下被严重地削弱或降低,即低温阻止了代谢途径的光保护机制的正常运转。 6.多酚物质在UV-B辐射或低温10/5℃条件下都能显著地累积,且在UV-B辐射和低温复合作用下增加尤其显著,表明多酚物质在两个温度生长条件下特别是低温条件下都参与了对UV-B辐射幼苗的保护。 7.在高温条件下仅仅SHUVB处理的幼苗TBARS含量显著增加,而低温10/5℃条件下两个UV-B辐射处理都非常显著地上升,说明与高温生长条件相比较,低温加重了UV-B辐射引起的氧化胁迫,低温10/5℃条件下幼苗多酚的增加以及抗氧化系统的部分增强都没有能阻止UV-B辐射对幼苗的伤害。

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We have carried out high contrast imaging of 70 young, nearby B and A stars to search for brown dwarf and planetary companions as part of the Gemini NICI Planet-Finding Campaign. Our survey represents the largest, deepest survey for planets around high-mass stars (≈1.5-2.5 M ☉) conducted to date and includes the planet hosts β Pic and Fomalhaut. We obtained follow-up astrometry of all candidate companions within 400 AU projected separation for stars in uncrowded fields and identified new low-mass companions to HD 1160 and HIP 79797. We have found that the previously known young brown dwarf companion to HIP 79797 is itself a tight (3 AU) binary, composed of brown dwarfs with masses 58$^{+21}_{-20}$ M Jup and 55$^{+20}_{-19}$ M Jup, making this system one of the rare substellar binaries in orbit around a star. Considering the contrast limits of our NICI data and the fact that we did not detect any planets, we use high-fidelity Monte Carlo simulations to show that fewer than 20% of 2 M ☉ stars can have giant planets greater than 4 M Jup between 59 and 460 AU at 95% confidence, and fewer than 10% of these stars can have a planet more massive than 10 M Jup between 38 and 650 AU. Overall, we find that large-separation giant planets are not common around B and A stars: fewer than 10% of B and A stars can have an analog to the HR 8799 b (7 M Jup, 68 AU) planet at 95% confidence. We also describe a new Bayesian technique for determining the ages of field B and A stars from photometry and theoretical isochrones. Our method produces more plausible ages for high-mass stars than previous age-dating techniques, which tend to underestimate stellar ages and their uncertainties.

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Recently the National Patient Safety Agency in the United Kingdom published a report entitled "Mitigating surgical risk in patients undergoing hip arthroplasty for fractures of the proximal femur". A total of 26 deaths had been reported to them when cement was used at hemiarthroplasty between October 2003 and October 2008. This paper considers the evidence for using cement fixation of a hemiarthroplasty in the treatment of hip fractures.

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The structure of the pseudo-merohedrally twinned crystal of the 1:1 proton-transfer compound of 5-sulfosalicylic acid (3-carboxy-4-hydroxybenzenesulfonic acid) with 4-aminopyridine: 4-aminopyridinium 3-carboxy-4-hydroxybenzenesulfonate sesquihydrate has been determined at 180 K and the hydrogen-bonding pattern is described. Crystals of the compound are monoclinic with space group P21/c, with unit cell dimensions a = 35.2589(8), b = 7.1948(1), c = 24.5851(5) Å, β = 110.373(2)o, and Z = 16. The monoclinic asymmetric unit comprises four cation-anion pairs and six water molecules of solvation with only the pyridinium cations having pseudo-symmetry as a result of inter-cation aromatic ring π-π stacking effects. Extensive hydrogen bonding gives a three-dimensional framework structure.

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The crystal structures of the proton-transfer compounds of 3,5-dinitrosalicylic acid (DNSA) with a series of aniline-type Lewis bases [aniline, 2-hydroxyaniline, 2-methoxyaniline, 3-methoxyaniline, 4-fluoroaniline, 4-chloroaniline and 2-aminoaniline] have been determined and their hydrogen-bonding systems analysed. All are anhydrous 1:1 salts: [(C6H8N)+(C7H3N2O7)-], (1), [(C6H8NO)+(C7H3N2O7)-], (2), [(C7H10NO)+(C7H3N2O7)-], (3), [(C7H10NO)+(C7H3N2O7)-], (4), [(C6H7FN)+(C7H3N2O7)-], (5), [(C6H7ClN)+(C7H3N2O7)-], (6), and [(C6H9N2)+(C7H3N2O7)-], (7) respectively. Crystals of 1 and 6 are triclinic, space group P-1 while the remainder are monoclinic with space group either P21/n (2, 4, 5 and 7) or P21 (3). Unit cell dimensions and contents are: for 1, a = 7.2027(17), b = 7.5699(17), c = 12.9615(16) Å, α = 84.464(14), β = 86.387(15), γ = 75.580(14)o, Z = 2; for 2, a = 7.407(3), b = 6.987(3), c = 27.653(11) Å, β = 94.906(7)o, Z = 4; for 3, a = 8.2816(18), b = 23.151(6), c = 3.9338(10), β = 95.255(19)o, Z = 2; for 4, a = 11.209(2), b = 8.7858(19), c = 15.171(3) Å, β = 93.717(4)o, Z = 4; for 5, a = 26.377(3), b = 10.1602(12), c = 5.1384(10) Å, β = 91.996(13)o, Z = 4; for 6, a = 11.217(3), b = 14.156(5), c = 4.860(3) Å, α = 99.10(4), β = 96.99(4), γ = 76.35(2)o, Z = 2; for 7, a = 12.830(4), b = 8.145(3), c = 14.302(4) Å, β = 102.631(6)o, Z = 4. In all compounds at least one primary linear intermolecular N+-H…O(carboxyl) hydrogen-bonding interaction is present which, together with secondary hydrogen bonding results in the formation of mostly two-dimensional network structures, exceptions being with compounds 4 and 5 (one-dimensional) and compound 6 (three-dimensional). In only two cases [compounds 1 and 4], are weak cation-anion or cation-cation π-π interactions found while weak aromatic C-H…O interactions are insignificant. The study shows that all compounds fit the previously formulated classification scheme for primary and secondary interactive modes for proton-transfer compounds of 3,5-dinitrosalicylic acid but there are some unusual variants.

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Two inorganic-organic hybrid framework iron phosphate-oxalates, I, [N2C4H12](0.5)[Fe-2(HPO4)(C2O4)(1.5)] and II, [Fe-2(OH2)PO4(C2O4)(0.5)] have been synthesized by hydrothermal means and the structures determined by X-ray crystallography. Crystal Data: compound I, monoclinic, spacegroup = P2(1)/c (No. 14), a=7.569(2) Angstrom, b=7.821(2) Angstrom, c=18.033(4) Angstrom, beta=98.8(1)degrees, V=1055.0(4) Angstrom(3), Z=4, M=382.8, D-calc=2.41 g cm(-3) MoK alpha, R-F=0.02; compound II, monoclinic, spacegroup=P2(1)/c (No. 14), a=10.240(1) b=6.375(3) Angstrom, 9.955(1) Angstrom, beta=117.3(1)degrees, V=577.4(1) Angstrom(3), Z=4, M=268.7, D-calc=3.09 g cm(-3) MoK alpha, R-F=0.03. These materials contain a high proportion of three-coordinated oxygens and [Fe2O9] dimeric units, besides other interesting structural features. The connectivity of Fe2O9 is entirely different in the two materials resulting in the formation of a continuous chain of Fe-O-Fe in II. The phosphate-oxalate containing the amine, I, forms well-defined channels. Magnetic susceptibility measurements show Fen to be in the high-spin state (t(2g)(4)e(g)(2)) in II, and in the intermediate-spin state (t(2g)(5)e(g)(1)) in I.

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Na+.C6HI209 P-, Mr=282.1, monoclinic, e2~, a=5-762(1), b=7.163(2), c=12.313(1)A, fl= 99.97 (1) °, U= 500.5 A 3, Z= 2, D m = 1.86, D x = 1.87 Mg m -s, Cu Ka, 2 = 1.5418 A, /a = 3-3 mm -1, F(000) = 292, T= 300 K, final R for 922 observed reflections is 0-042. The phosphate ester bond, P-O(6), is 1.575 (5)A, slightly shorter than the P~O bond in monopotassium phosphoenolpyruvate [1.612 (6) A] [Hosur & Viswamitra (1981). Acta Cryst. B37, 839-843]. The pyranose sugar ring takes a 4C 1 chair conformation. The conformation about the exocyclic C(5)-C(6) bond is gauche-trans. The endocyclic C-O bonds in the glucose ring are nearly equal with C(5)-O(5) = 1.435 (8) and C(1)-O(5) = 1.436 (9) A. The sodium ion has seven near neighbours within a distance of 2.9 A. The crystal structure is stabilized by hydrogen bonds between the O atoms of symmetryrelated molecules.

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l-Lysine acetate crystallises in the monoclinic space group P21 with a = 5.411 (1), b = 7.562(1), c= l2.635(2) Å and β = 91.7(1). The crystal structure was solved by direct methods and refined to an R value of 0.049 using the full matrix least squares method. The conformation and the aggregation of lysine molecules in the structure are similar to those found in the crystal structure of l-lysine l-aspartate. A conspicuous similarity between the crystal structures of l-arginine acetate and l-lysine acetate is that in both cases the strongly basic side chain, although having the largest pK value, interacts with the weakly acidic acetate group leaving the α-amino and the α-carboxylate groups to take part in head-to-tail sequences. These structures thus indicate that electrostatic effects are strongly modulated by other factors so as to give rise to head-to-tail sequences which have earlier been shown to be an almost universal feature of amino acid aggregation in the solid state.

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Mr = 248, monoclinic, P21/n, a = 12.028 (2), b=7.168(2), c= 15.187(5)A, fl=91.88(2) °, Z= 4, V= 1308.6,~3, Din= 1.26, Dx= 1.263 Mgm -3, 2 (Cu Ka) = 1.5418 .A, g = 0.86 mm -1, F(000) = 536, T= 293 K. Final R = 5.6% for 2120 observed reflexions. Owing to the push-pull effect, the C=C bond distance is as long as 1.464 (2)/k with the twist angle about the bond 62.6.

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CsHsN204, M r = 197.2, monoclinic, P21/e , a= 7.818 (2), b= 7.589 (2), e= 14.790 (2)A, t= 98.43 (2) °, V= 868.02/k 3, Z = 4, D m = 1.506 (3), Dx= 1.501Mgm -3, MoKa, 2=0.7107/~, #= 0-79 mm -1, F(000) = 408, T= 426 (1) K, final R = 0.0507 for 798 observed reflections [I_> 2e(/)]. The molecules are hydrogen bonded: N-H...O = 2.886 (3), N--H = 0.97 (7), H--O = 1.92 (6) A, N-- H...O angle = 175.5 (8) °.

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M r = 251.34, monoclinic, P21/n, a =14.626 (3), b= 7.144 (1), c= 11.996 (2)\AA \betat=90.03 (2) °, V= 1253.4 (6) \AA 3, Z = 4, Dm= 1.326 (3),Dx=1.331(3)gcm -3, MoKat, \lambda = 0.7107 )\AA , \mu=3.51 cm -3, F(000) = 528.0, T-- 293 K, R -- 3.5% for1455 significant reflections. Of particular interest is an intramolecular attractive interaction between the sulphur and oxygen atoms with an S...O distance of 2.658 (3)\AA, in which the oxygen atom appears to actas a nucleophile.