939 resultados para Dyson, Matt
Resumo:
L-R: Tom Brenner, Don Hill, coach Matt Mann, Wally Jeffries, Burwell (Bumpy) Jones
Resumo:
Front Row, Left to Right: Thomas DeMassa, James Sytek, Jack Zachary, Robert Wojcik, Jerry Leith, Harry Newman, Jr., Dave Brown, James McPherson, Alvin Groce, Grant Walls, John Halstead, Joseph Brefeld, Richard Syring, Phil Barger, Wilfrid Grein, John Galarneault.
Second Row: Coach Don Dufek, John Batsakes, Paul Poulos, Fred Olm, Dennis Fitzgerald, Jim Byers, Doug Oppman, Robert Ptacek, John Herrnstein, Gary Prahst, Walt Johnson, Gerald Marciniak, Willie Smith, Anthony Rio, Michael Dupay, Mike Fillichio, Bob Johnson, Jim Dickey, Coach Matt Patanelli.
Third Row: Coach Jack Blott, Coach Bob Hollway, James Gray, Maynard Stetten, Gordon Morrow, Eugene Sisinyak, Guy Curtis, B. Lee Hall, Darrell Harper, Jared Bushong, Alex Callahan, Wesley Maki, Donald Kolcheff, Fred Julian, George Genyk, Gerald Smith, Robert Swanson, Willerfred Wilson, Erwin Crownley, Coach Ben Oosterbaan.
Back Row: Coach Wally Weber, Reid Bushong, Gary McNitt, Bill Stein, Tom Jobson, Donald Hannah, Gary Kane, John Walker, Willard Hildebrand, Paul Raeder, Darrell Thorpe, Daniel Snow, Thomas Kerr, Lovell Farris, David Palomaki, Bradley Myers, Donald Deskins, Arthur Lazik, John Spidel, Keith Cowan, Henry Stuart, Coach "Bump" Elliott.
Resumo:
Back Row: Cedric Sweet, Franklin Lett, Steve Remias, Carl Carr, Russ Oliver, captain Thomas Austin, Robert Johnson, Willard Hildebrandt, Edward Stone, Michael Savage, Thomas Oyler, Harry Wright, Joe Fisher, Jack Liffiton, John Viergever, Herman Everhardus, Willis Ward, Matt Patanelli, Robert Graper
Middle Row: John Mumford, James Kidston, William Borgmann, Chester Beard, Howard Triplehorn, Vincent Pope, Ernest Pederson, Joseph Ellis, Robert Amrine, Russell Fuog, Stanton Schuman, Vincent Aug, Winfred Nelson, John Regeczi
Front Row: John Connolly, Jesse Garber, David Barnett, John Rieck, Frank Bissell, Eli Soodik, William Renner, Richard James, Ferris Jennings, Harry Pillinger, Harry Lutomski, George Bolas, Charles Brandman, Gerald Ford
Resumo:
Back Row: Cedric Sweet, Franklin Lett, Steve Remias, Carl Carr, Russ Oliver, captain Thomas Austin, Robert Johnson, Willard Hildebrandt, Edward Stone, Michael Savage, Thomas Oyler, Harry Wright, Joe Fisher, Jack Liffiton, John Viergever, Herman Everhardus, Willis Ward, Matt Patanelli, Robert Graper
Middle Row: John Mumford, James Kidston, William Borgmann, Chester Beard, Howard Triplehorn, Vincent Pope, Ernest Pederson, Joseph Ellis, Robert Amrine, Russell Fuog, Stanton Schuman, Vincent Aug, Winfred Nelson, John Regeczi
Front Row: John Connolly, Jesse Garber, David Barnett, John Rieck, Frank Bissell, Eli Soodik, William Renner, Richard James, Ferris Jennings, Harry Pillinger, Harry Lutomski, George Bolas, Charles Brandman, Gerald Ford
Resumo:
Solomon Sobsey, Harold Floersch, Donald Siegel, Edward Greenwald, Cedric Sweet, John Brennan, Matt Patanelli, Seymour Rosenthall, Melvin Kramer, Fred Jahnke, John Jordan, Norman Nickerson, Arthur Valpey, Earle Luby, George Shakarian, Elmer Gedeon, Dan Smick, Chris Everhardus, Donald Paquette
Middle Row: Edward Stanton, Alex Loiko, John Smithers, Fred Olds, Joseph Rinaldi, George Maurer, George Marzonie, Robert Cooper, Forrest Jordan, Frederick Ziem, Ernest Pederson, James Lincoln, William Barclay, Douglas Farmer, C. Stark Ritchie, Clarence VandeWater, Martin Mark, Ralph Heikkinen
Front Row: Robert Campbell, Frank Bissell, Ferris Jennings, Charles Gray, Norm Purucker, Jerome Belsky, Chester Stabovitz, Kenneth Frost, Robert Curren, R. Wallace Hook, Joseph Barassa, Lilburn Ochs, Louis Levine, Blair Philips, Jesse Garber, Robert Piotrowski, James Barnett
Resumo:
Top Row: Ted Kress, Dave Williams, William McKinley, Larry Cox, Dave Hill, Dick Kolesar, Van Schoick, Earl Johnson, Bob Ames.
6th Row: Tony Branoff, Ed Hickey, Don Bennett, Dick Vorenkamp, Tom Hendricks, Doug Murray, Charles Ritter, Mike Orend, Carl Kamhout, Jim Kirby, Joe Krahl.
5th Row: Don Dugger, Jack Wheeler, Wilbur Brown, Jerry Gonser, Bob Sriver, Jim Bates, Ray Donohoe, Dick Strozewski, Dave Rentschler, John Kuchka, George Corey, Phil Endres.
4h Row: Gerry Williams, Gordon Barnes, Edgar Meads, Charles Krahnke, Fred Baer, Stanley Knickerbocker, Jim Fox, John Peckham, John Morrow, Dick Rex, Coach J. T. White.
3rd Row: Coach Don Robinson, Don Drake, Joe Shomsky, Lou Baldacci, Salvatore DiMucci, George Dutter, Ray Kenaga, George Muellich, Jim Bowman, Ted Cachey, Coach Bill Orwig.
2nd Row: Cliff Keen, Dean Ludwig, Duncan McDonald, Ken Shields, Peri Gagalis, Pete Wolgast, Bob Milligan, Ron Geyer, Dick Beison, Dan Cline, Art Walker, Coach Matt Patanelli.
Front Row: Wally Weber, John Veselenak, Tad Stanford, Gene Knutson, Dick Balzhiser, Captain Dick O'Shaughnessy; Head Coach Bennie Oosterbaan; Bob Marion, Bob Topp, Ray VanderZeyde, Ron Williams, Jim Balog, Jack Blott.
Resumo:
There are TWO versions of this - the initial file (pieced together from two scans) AND a version that has been enhanced by Matt Adair to darken the signatures and make them more legible. They share the same hs#, but the second version includes the suffix "enhanced".
Resumo:
Includes index.
Resumo:
At head of title: State of California. James Rolph, jr., governor. Matt I. Sullivan, chairman.
Resumo:
We have discovered a new type of galaxy in the Fornax Cluster: 'ultra-compact' dwarfs (UCDs). The UCDs are unresolved in ground-based imaging and have spectra typical of old stellar systems. Although the UCDs resemble overgrown globular clusters, based on VLT UVES echelle spectroscopy, they appear to be dynamically distinct systems with higher internal velocity dispersions and M/L ratios for a given luminosity than Milky Way or M31 globulars. Our preferred explanation for their origin is that they are the remnant nuclei of dwarf elliptical galaxies which have been tidally stripped, or 'threshed' by repeated encounters with the central cluster galaxy, NGC1399. If correct, then tidal stripping of nucleated dwarfs to form UCDs may, over a Hubble time, be an important source of the plentiful globular cluster population in the halo of NGC1399, and, by implication, other cD galaxies. In this picture, the dwarf elliptical halo contents, up to 99% of the original dwarf luminosity, contribute a significant fraction of the populations of intergalactic stars, globulars, and gas in galaxy clusters.
Resumo:
Background and Aims Quercus petraea colonized Ireland after the last glaciation from refugia on mainland Europe. Deforestation. however. beginning in Neolithic times, has resulted in small, scattered forest fragments, now covering less than 12 000 ha. Methods Plastid (three fragments) and microsatellite variation (13 loci) were characterized in seven Irish populations sampled along a north-south gradient. Using Bayesian approaches and Wright's F-statistics, the effects of colonization and fragmentation on the genetic structure and mating patterns of extant oak populations were investigated. Key-Results All Populations possessed cytotypes common to the Iberian Peninsula. Despite the distance from the refugial core and the extensive deforestation in Ireland, nuclear genetic variation was high and comparable to mainland Europe. Low population differentiation was observed within Ireland and populations showed no evidence for isolation by distance. As expected of a marker with an effective Population size of one-quarter relative to the nuclear genome, plastid variation indicated higher differentiation. Individual inbreeding coefficients indicated high levels of outcrossing. Conclusions Consistent with a large effective Population size in the historical migrant gene pool and/or with high gene flow among populations, high within-population diversity and low population differentiation was observred within Ireland. It is proposed that native Q. petraea populations in Ireland share a common phylogeographic history and that the present genetic structure does not reflect founder effects. (C) 2004 Annals of Botany Company.
Resumo:
English School approaches to international politics, which focus on the idea of an international society of states bound together by shared rules and norms, have not paid significant explicit attention to the study of security in international relations. This is curious given the centrality of security to the study of world politics and the recent resurgence of English School scholarship in general. This article attempts to redress this gap by locating and explicating an English School discourse of security. We argue here that there is indeed an English School discourse of security, although an important internal distinction exists here between pluralist and solidarist accounts, which focus on questions of order and justice in international society respectively. In making this argument, we also seek to explore the extent to which emerging solidarist accounts of security serve to redress the insecurity of security in international relations: the tendency of traditional security praxes to privilege the state in ways that renders individuals insecure.
Resumo:
Poly(3-hydroxybutyrate-co-3-hydroxyvalerate) (PHBV) melt processed disks and solvent cast films were modified by graft co-polyinerization with acrylic acid (AAc) in methanol solution at ambient temperature using gamma irradiation (dose rate of 4.5 kGy/h). To assess the presence of carboxylic acid groups on the surface, reaction with pentafluorophenol was performed prior to X-ray photoelectron spectroscopy analysis. The grafting yield for all samples increased with monomer concentration (2-15%), and for the solvent cast films, it also increased with dose (2-9 kGy). However, the grafting yield of the melt processed disks was largely independent of the radiation dose (2-8 kGy). Toluidine blue was used to stain the modified materials facilitating, visual information about the extent of carboxylic acid functionalization and depth penetration of the grafted copolymer. Covalent linking of glucosamine to the functionalized surface was achieved using carbodimide chemistry verifying that the modified substrates are suitable for biomolecule attachment.
Resumo:
The sedimentation rate of sand grains in the hindered settling regime has been considered to assess particle shape effects. The behaviour of various particulate systems involving sand has been compared with the widely used Richardson-Zaki expression. The general form of the expression is found to hold, in as much as remaining as a suitable means to describe the hindered settling of irregular particles. The sedimentation exponent n in the Richardson-Zaki expression is found to be significantly larger for natural sand grains than for regular particles. The hindered settling effect is therefore greater, leading to lower concentration gradients than expected. The effect becomes more pronounced with increasing particle irregularity. At concentrations around 0.4, the hindered settling velocity of fine and medium natural sands reduces to about 70% of the value predicted using existing empirical expressions for n. Using appropriate expressions for the fluidization velocity and the clear water settling velocity, a simple method is discussed to evaluate the sedimentation exponent and to determine the hindered settling effect for sands of various shapes.