5,343 research outputs found

    Problems in Development of Nationalism in India

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    An analysis of the dynamics of development of significant strands within the Indian nationalist movement prior to World War I

    Thermal conductivity of heterogeneous mixtures and lunar soils

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    The theoretical evaluation of the effective thermal conductivity of granular materials is discussed with emphasis upon the heat transport properties of lunar soil. The following types of models are compared: probabilistic, parallel isotherm, stochastic, lunar, and a model based on nonlinear heat flow system synthesis

    The replacement histone H2A.Z in a hyperacetylated form is a feature of active genes in the chicken

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    The replacement histone H2A.Z is variously reported as being linked to gene expression and preventing the spread of heterochromatin in yeast, or concentrated at heterochromatin in mammals. To resolve this apparent dichotomy, affinity-purified antibodies against the N-terminal region of H2A.Z, in both a triacetylatedandnon- acetylatedstate, areusedin native chromatin immmuno-precipitation experiments with mononucleosomes from three chicken cell types. The hyperacetylated species concentrates at the 50 end of active genes, both tissue specific and housekeeping but is absent from inactive genes, while the unacetylated form is absent from both active and inactive genes. A concentration of H2A.Z is also found at insulators under circumstances implying a link to barrier activity but not to enhancer blocking. Although acetylated H2A.Z is widespread throughout the interphase genome, at mitosis its acetylation is erased, the unmodified form remaining. Thus, although H2A.Z may operate as an epigenetic marker for active genes, its N-terminal acetylation does not

    The replacement histone H2A.Z in a hyperacetylated form is a feature of active genes in the chicken

    Get PDF
    The replacement histone H2A.Z is variously reported as being linked to gene expression and preventing the spread of heterochromatin in yeast, or concentrated at heterochromatin in mammals. To resolve this apparent dichotomy, affinity-purified antibodies against the N-terminal region of H2A.Z, in both a triacetylatedandnon- acetylatedstate, areusedin native chromatin immmuno-precipitation experiments with mononucleosomes from three chicken cell types. The hyperacetylated species concentrates at the 50 end of active genes, both tissue specific and housekeeping but is absent from inactive genes, while the unacetylated form is absent from both active and inactive genes. A concentration of H2A.Z is also found at insulators under circumstances implying a link to barrier activity but not to enhancer blocking. Although acetylated H2A.Z is widespread throughout the interphase genome, at mitosis its acetylation is erased, the unmodified form remaining. Thus, although H2A.Z may operate as an epigenetic marker for active genes, its N-terminal acetylation does not

    Structural and chemical requirements for histidine phosphorylation by the chemotaxis kinase CheA

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    The CheA histidine kinase initiates the signal transduction pathway of bacterial chemotaxis by autophosphorylating a conserved histidine on its phosphotransferase domain (P1). Site-directed mutations of neighboring conserved P1 residues (Glu-67, Lys-48, and His-64) show that a hydrogen-bonding network controls the reactivity of the phospho-accepting His (His-45) in Thermotoga maritima CheA. In particular, the conservative mutation E67Q dramatically reduces phospho-transfer to P1 without significantly affecting the affinity of P1 for the CheA ATP-binding domain. High resolution crystallographic studies revealed that although all mutants disrupt the hydrogen-bonding network to varying degrees, none affect the conformation of His-45. N-15-NMR chemical shift studies instead showed that Glu-67 functions to stabilize the unfavored (NH)-H-delta 1 tautomer of His-45, thereby rendering the N-epsilon 2 imidazole unprotonated and well positioned for accepting the ATP phosphoryl group

    Magellan/M2FS Spectroscopy of Galaxy Clusters: Stellar Population Model and Application to Abell 267

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    We report the results of a pilot program to use the Magellan/M2FS spectrograph to survey the galactic populations and internal kinematics of galaxy clusters. For this initial study, we present spectroscopic measurements for 223223 quiescent galaxies observed along the line of sight to the galaxy cluster Abell 267 (z∼0.23z\sim0.23). We develop a Bayesian method for modeling the integrated light from each galaxy as a simple stellar population, with free parameters that specify redshift (vlos/cv_\mathrm{los}/c) and characteristic age, metallicity ([Fe/H]\mathrm{[Fe/H]}), alpha-abundance ([α/Fe][\alpha/\mathrm{Fe}]), and internal velocity dispersion (σint\sigma_\mathrm{int}) for individual galaxies. Parameter estimates derived from our 1.5-hour observation of A267 have median random errors of σvlos=20 km s−1\sigma_{v_\mathrm{los}}=20\ \mathrm{km\ s^{-1}}, σAge=1.2 Gyr\sigma_{\mathrm{Age}}=1.2\ \mathrm{Gyr}, $\sigma_{\mathrm{[Fe/H]}}=0.11\ \mathrm{dex},, \sigma_{[\alpha/\mathrm{Fe}]}=0.07\ \mathrm{dex},and, and \sigma_{\sigma_\mathrm{int}}=20\ \mathrm{km\ s^{-1}}$. In a companion paper, we use these results to model the structure and internal kinematics of A267.Comment: 16 pages, 11 figures, accepted for publication in The Astronomical Journa

    NGC 1866: First Spectroscopic Detection of Fast Rotating Stars in a Young LMC Cluster

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    High-resolution spectroscopic observations were taken of 29 extended main sequence turn-off (eMSTO) stars in the young (∼\sim200 Myr) LMC cluster, NGC 1866 using the Michigan/Magellan Fiber System and MSpec spectrograph on the Magellan-Clay 6.5-m telescope. These spectra reveal the first direct detection of rapidly rotating stars whose presence has only been inferred from photometric studies. The eMSTO stars exhibit H-alpha emission (indicative of Be-star decretion disks), others have shallow broad H-alpha absorption (consistent with rotation ≳\gtrsim 150 km s−1^{-1}), or deep H-alpha core absorption signaling lower rotation velocities (≲ \lesssim 150 km s−1^{-1} ). The spectra appear consistent with two populations of stars - one rapidly rotating, and the other, younger and slowly rotating.Comment: 9 pages, 4 figures, Accepted for publication in ApJ Letter

    Market-oriented interventions and climate resilience in dryland agro-pastoralism

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    European Unio
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