TY - JOUR A1 - Arnison, Paul G. A1 - Bibb, Mervyn J. A1 - Bierbaum, Gabriele A1 - Bowers, Albert A. A1 - Bugni, Tim S. A1 - Bulaj, Grzegorz A1 - Camarero, Julio A. A1 - Campopiano, Dominic J. A1 - Challis, Gregory L. A1 - Clardy, Jon A1 - Cotter, Paul D. A1 - Craik, David J. A1 - Dawson, Michael A1 - Dittmann-Thünemann, Elke A1 - Donadio, Stefano A1 - Dorrestein, Pieter C. A1 - Entian, Karl-Dieter A1 - Fischbach, Michael A. A1 - Garavelli, John S. A1 - Goeransson, Ulf A1 - Gruber, Christian W. A1 - Haft, Daniel H. A1 - Hemscheidt, Thomas K. A1 - Hertweck, Christian A1 - Hill, Colin A1 - Horswill, Alexander R. A1 - Jaspars, Marcel A1 - Kelly, Wendy L. A1 - Klinman, Judith P. A1 - Kuipers, Oscar P. A1 - Link, A. James A1 - Liu, Wen A1 - Marahiel, Mohamed A. A1 - Mitchell, Douglas A. A1 - Moll, Gert N. A1 - Moore, Bradley S. A1 - Mueller, Rolf A1 - Nair, Satish K. A1 - Nes, Ingolf F. A1 - Norris, Gillian E. A1 - Olivera, Baldomero M. A1 - Onaka, Hiroyasu A1 - Patchett, Mark L. A1 - Piel, Jörn A1 - Reaney, Martin J. T. A1 - Rebuffat, Sylvie A1 - Ross, R. Paul A1 - Sahl, Hans-Georg A1 - Schmidt, Eric W. A1 - Selsted, Michael E. A1 - Severinov, Konstantin A1 - Shen, Ben A1 - Sivonen, Kaarina A1 - Smith, Leif A1 - Stein, Torsten A1 - Suessmuth, Roderich D. A1 - Tagg, John R. A1 - Tang, Gong-Li A1 - Truman, Andrew W. A1 - Vederas, John C. A1 - Walsh, Christopher T. A1 - Walton, Jonathan D. A1 - Wenzel, Silke C. A1 - Willey, Joanne M. A1 - van der Donk, Wilfred A. T1 - Ribosomally synthesized and post-translationally modified peptide natural products overview and recommendations for a universal nomenclature JF - Natural product reports : a journal of current developments in bio-organic chemistry N2 - This review presents recommended nomenclature for the biosynthesis of ribosomally synthesized and post-translationally modified peptides (RiPPs), a rapidly growing class of natural products. The current knowledge regarding the biosynthesis of the >20 distinct compound classes is also reviewed, and commonalities are discussed. Y1 - 2013 U6 - https://doi.org/10.1039/c2np20085f SN - 0265-0568 VL - 30 IS - 1 SP - 108 EP - 160 PB - Royal Society of Chemistry CY - Cambridge ER - TY - JOUR A1 - Richardson, Noel D. A1 - Russell, Christopher M. P. A1 - St-Jean, Lucas A1 - Moffat, Anthony F. J. A1 - St-Louis, Nicole A1 - Shenar, Tomer A1 - Pablo, Herbert A1 - Hill, Grant M. A1 - Ramiaramanantsoa, Tahina A1 - Corcoran, Michael A1 - Hamuguchi, Kenji A1 - Eversberg, Thomas A1 - Miszalski, Brent A1 - Chene, Andre-Nicolas A1 - Waldron, Wayne A1 - Kotze, Enrico J. A1 - Kotze, Marissa M. A1 - Luckas, Paul A1 - Cacella, Paulo A1 - Heathcote, Bernard A1 - Powles, Jonathan A1 - Bohlsen, Terry A1 - Locke, Malcolm A1 - Handler, Gerald A1 - Kuschnig, Rainer A1 - Pigulski, Andrzej A1 - Popowicz, Adam A1 - Wade, Gregg A. A1 - Weiss, Werner W. T1 - The variability of the BRITE-est Wolf-Rayet binary, gamma(2) Velorum-I. Photometric and spectroscopic evidence for colliding winds JF - Monthly notices of the Royal Astronomical Society N2 - We report on the first multi-colour precision light curve of the bright Wolf-Rayet binary gamma(2) Velorum, obtained over six months with the nanosatellites in the BRITE-Constellation fleet. In parallel, we obtained 488 high-resolution optical spectra of the system. In this first report on the data sets, we revise the spectroscopic orbit and report on the bulk properties of the colliding winds. We find a dependence of both the light curve and excess emission properties that scales with the inverse of the binary separation. When analysing the spectroscopic properties in combination with the photometry, we find that the phase dependence is caused only by excess emission in the lines, and not from a changing continuum. We also detect a narrow, high-velocity absorption component from the He perpendicular to lambda 5876 transition, which appears twice in the orbit. We calculate smoothed-particle hydrodynamical simulations of the colliding winds and can accurately associate the absorption from He perpendicular to to the leading and trailing arms of the wind shock cone passing tangentially through our line of sight. The simulations also explain the general strength and kinematics of the emission excess observed in wind lines such as C III lambda 5696 of the system. These results represent the first in a series of investigations into the winds and properties of gamma(2) Velorum through multi-technique and multi-wavelength observational campaigns. KW - stars: early type KW - stars: individual: gamma(2) Vel KW - stars: mass loss KW - stars: winds KW - outflows KW - stars: Wolf-Rayet Y1 - 2017 U6 - https://doi.org/10.1093/mnras/stx1731 SN - 0035-8711 SN - 1365-2966 VL - 471 SP - 2715 EP - 2729 PB - Oxford Univ. Press CY - Oxford ER - TY - JOUR A1 - Jones, Geraint H. A1 - Arridge, Christopher S. A1 - Coates, Andrew J. A1 - Lewis, Gethyn R. A1 - Kanani, Sheila A1 - Wellbrock, Anne A1 - Young, David T. A1 - Crary, Frank J. A1 - Tokar, Robert L. A1 - Wilson, R. J. A1 - Hill, Thomas W. A1 - Johnson, Robert E. A1 - Mitchell, Donald G. A1 - Schmidt, Jürgen A1 - Kempf, Sascha A1 - Beckmann, Uwe A1 - Russell, Christopher T. A1 - Jia, Y. D. A1 - Dougherty, Michele K. A1 - Waite, J. Hunter A1 - Magee, Brian A. T1 - Fine jet structure of electrically charged grains in Enceladus' plume N2 - By traversing the plume erupting from high southern latitudes on Saturn's moon Enceladus, Cassini orbiter instruments can directly sample the material therein. Cassini Plasma Spectrometer, CAPS, data show that a major plume component comprises previously-undetected particles of nanometer scales and larger that bridge the mass gap between previously observed gaseous species and solid icy grains. This population is electrically charged both negative and positive, indicating that subsurface triboelectric charging, i.e., contact electrification of condensed plume material may occur through mutual collisions within vents. The electric field of Saturn's magnetosphere controls the jets' morphologies, separating particles according to mass and charge. Fine-scale structuring of these particles' spatial distribution correlates with discrete plume jets' sources, and reveals locations of other possible active regions. The observed plume population likely forms a major component of high velocity nanometer particle streams detected outside Saturn's magnetosphere. Y1 - 2009 UR - http://www.agu.org/journals/gl/ U6 - https://doi.org/10.1029/2009gl038284 SN - 0094-8276 ER - TY - JOUR A1 - Meier, Patrick A1 - Kriegel, Hendrik A1 - Motschmann, Uwe A1 - Schmidt, Jürgen A1 - Spahn, Frank A1 - Hill, Thomas W. A1 - Dong, Yaxue A1 - Jones, Geraint H. T1 - A model of the spatial and size distribution of Enceladus' dust plume JF - Planetary and space science KW - Enceladus KW - Plume KW - Nanograins KW - Cassini KW - Tail Y1 - 2014 U6 - https://doi.org/10.1016/j.pss.2014.09.016 SN - 0032-0633 VL - 104 SP - 216 EP - 233 PB - Elsevier CY - Oxford ER - TY - JOUR A1 - Meier, Patrick A1 - Motschmann, Uwe A1 - Schmidt, Jurgen A1 - Spahn, Frank A1 - Hill, Thomas W. A1 - Dong, Yaxue A1 - Jones, Geraint H. A1 - Kriegel, Hendrik T1 - Modeling the total dust production of Enceladus from stochastic charge equilibrium and simulations JF - Planetary and space science KW - Enceladus KW - Plume KW - Nanograin charge KW - CAPS Y1 - 2015 U6 - https://doi.org/10.1016/j.pss.2015.10.002 SN - 0032-0633 VL - 119 SP - 208 EP - 221 PB - Elsevier CY - Oxford ER -