一株软骨霉状菌的纯化方法

从武夷山的一枯枝上分离得到了一株稀有软骨霉状菌,在培养过程中发现,该株黏细菌在人工培养基上只有在与一种未知的细菌共培养的状态下才能长出典型的子实体并保持菌种的活力.然而要从共培养的菌落中纯化这株黏细菌,使用常规的黏细菌纯化技术几乎是不可能.在这种情况下对伴生细菌进行16SrDNA菌种鉴定,再根据鉴定为施氏假单胞菌(Ps...     

Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars

Red giants are evolved stars that have exhausted the supply of hydrogen in their cores and instead burn hydrogen in a surrounding shell. Once a red giant is sufficiently evolved, the helium in the core also undergoes fusion. Outstanding issues in our understanding of red giants include uncertainties in the amount of mass lost at the surface before helium ignition and the amount of internal mixing from rotation and other processes. Progress is hampered by our inability to distinguish between red giants burning helium in the core and those still only burning hydrogen in a shell. Asteroseismology offers a way forward, being a powerful tool for probing the internal structures of stars using their natural oscillation frequencies. Here we report observations of gravity-mode period spacings in red giants that permit a distinction between evolutionary stages to be made. We use high-precision photometry obtained by the Kepler spacecraft over more than a year to measure oscillations in several hundred red giants. We find many stars whose dipole modes show sequences with approximately regular period spacings. These stars fall into two clear groups, allowing us to distinguish unambiguously between hydrogen-shell-burning stars (period spacing mostly ～ 50 seconds) and those that are also burning helium (period spacing ～ 100 to 300 seconds).     

A closely packed system of low-mass, low-density planets transiting Kepler-11

When an extrasolar planet passes in front of (transits) its star, its radius can be measured from the decrease in starlight and its orbital period from the time between transits. Multiple planets transiting the same star reveal much more: period ratios determine stability and dynamics, mutual gravitational interactions reflect planet masses and orbital shapes, and the fraction of transiting planets observed as multiples has implications for the planarity of planetary systems. But few stars have more than one known transiting planet, and none has more than three. Here we report Kepler spacecraft observations of a single Sun-like star, which we call Kepler-11, that reveal six transiting planets, five with orbital periods between 10 and 47?days and a sixth planet with a longer period. The five inner planets are among the smallest for which mass and size have both been measured, and these measurements imply substantial envelopes of light gases. The degree of coplanarity and proximity of the planetary orbits imply energy dissipation near the end of planet formation.     

Mutations in the RNA exosome component gene EXOSC3 cause pontocerebellar hypoplasia and spinal motor neuron degeneration

RNA exosomes are multi-subunit complexes conserved throughout evolution and are emerging as the major cellular machinery for processing, surveillance and turnover of a diverse spectrum of coding and noncoding RNA substrates essential for viability. By exome sequencing, we discovered recessive mutations in EXOSC3 (encoding exosome component 3) in four siblings with infantile spinal motor neuron disease, cerebellar atrophy, progressive microcephaly and profound global developmental delay, consistent with pontocerebellar hypoplasia type 1 (PCH1; MIM 607596). We identified mutations in EXOSC3 in an additional 8 of 12 families with PCH1. Morpholino knockdown of exosc3 in zebrafish embryos caused embryonic maldevelopment, resulting in small brain size and poor motility, reminiscent of human clinical features, and these defects were largely rescued by co-injection with wild-type but not mutant exosc3 mRNA. These findings represent the first example of an RNA exosome core component gene that is responsible for a human disease and further implicate dysregulation of RNA processing in cerebellar and spinal motor neuron maldevelopment and degeneration.     

Generation of functional insulin-producing cells in the gut by Foxo1 ablation

Restoration of regulated insulin secretion is the ultimate goal of therapy for type 1 diabetes. Here, we show that, unexpectedly, somatic ablation of Foxo1 in Neurog3(+) enteroendocrine progenitor cells gives rise to gut insulin-positive (Ins(+)) cells that express markers of mature β cells and secrete bioactive insulin as well as C-peptide in response to glucose and sulfonylureas. Lineage tracing experiments showed that gut Ins(+) cells arise cell autonomously from Foxo1-deficient cells. Inducible Foxo1 ablation in adult mice also resulted in the generation of gut Ins(+) cells. Following ablation by the β-cell toxin streptozotocin, gut Ins(+) cells regenerate and produce insulin, reversing hyperglycemia in mice. The data indicate that Neurog3(+) enteroendocrine progenitors require active Foxo1 to prevent differentiation into Ins(+) cells. Foxo1 ablation in gut epithelium may provide an approach to restore insulin production in type 1 diabetes.     

RhoA/Rho激酶在大鼠阴茎勃起机制中的调节作用

一般认为一氧化氮（nitric oxide,NO）释放增加促进小动脉和海绵体平滑肌舒张是导致男性阴茎勃起的主要机制。研究发现内源性血管收缩因子对维持阴茎萎状态有重要作用。应用大鼠模型活体检测使用Y-27632拮抗Rho-激酶活性后对阴茎勃起生理机制的影响;应用免疫转印技术检测 阴茎海绵体内RhoA和Rho激酶蛋白的表达。结果显示在大鼠海绵体组织内有内源性RhoA和Rho激酶蛋白的表达和存在;Y-27632海绵体内注射阻滞RhoA/Rho激酶活性使ICP和CCP/MAP比值明显升高;局部小剂量应用Y-27632对MAP没有明显影响;Y-27632可增强系列电刺激引起的由NO介导的CCP/MAP比值的增加;NO合成酶和鸟苷酸环化酶抑制剂的作用不能阻滞RhoA/Rho激酶抑制剂对大鼠阴茎海绵体平滑肌的松弛作用和CCP/MAP的增加。说明RhoA/Rho激酶信号系统发挥了维持海绵体萎软状态重要作用,这是与NO介导途径不同的阴茎勃起生理调节机制。RhoA/Rho激酶抑制剂可能是ED治疗的新领域新方法。     

Mutations in a new member of the chromodomain gene family cause CHARGE syndrome

CHARGE syndrome is a common cause of congenital anomalies affecting several tissues in a nonrandom fashion. We report a 2.3-Mb de novo overlapping microdeletion on chromosome 8q12 identified by array comparative genomic hybridization in two individuals with CHARGE syndrome. Sequence analysis of genes located in this region detected mutations in the gene CHD7 in 10 of 17 individuals with CHARGE syndrome without microdeletions, accounting for the disease in most affected individuals.