Results 71 to 80 of about 9,409 (89)
Structure and dynamics of candidate O star bubbles in N44 [PDF]
, 2002 peer reviewedDynamical studies of superbubbles and Wolf-Rayet ring nebulae show discrepancies from the standard adiabatic model for windblown bubbles. We therefore study the physical properties and kinematics of three candidate bubbles blown by single O ...
Smith, R. C. +5 more
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Strongly base-paracompact spaces [PDF]
, 2003 summary:A space $X$ is said to be {\it strongly base-paracompact\/} if there is a basis $\Cal B$ for $X$ with $|\Cal B|=w(X)$ such that every open cover of $X$ has a star-finite open refinement by members of $\Cal B$.
Porter, John E.
core +1 more source
Stable homotopy groups of spheres. [PDF]
Proc Natl Acad Sci U S A, 2020 Isaksen DC, Wang G, Xu Z.
europepmc +1 more source
Properties of strongly star shaped cones
, 2007 In problems of vector optimization, with preferences that are not necessarily a pre-order relation, the strongly star shaped cones are very important in order to get a scalarization of these problems.
Morales-Silva, Daniel
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Interfaces in Numerical Relativistic hydrodynamics
, 2010 This thesis investigates numerical techniques for modelling sharp interfacesbetween relativistic fluids. The motivation for this work lies in obtaining accuratemodels of neutron star interiors for use in multidimensional simulationsin general relativity.
Millmore, Stephen Timothy
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AN EXAMPLE OF USING STAR COMPLEMENTS IN CLASSIFYING STRONGLY REGULAR GRAPHS ∗
, 2014 In this paper we show how the star complement technique can be used to reprove the result of Wilbrink and Brouwer that the strongly regular graph with parameters (57, 14, 1, 4) does not exist.
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Signals of the QCD Phase Transition in the Heavens
, 2007 The modern phase diagram of strongly interacting matter reveals a rich structure at high-densities due to phase transitions related to the chiral symmetry of quantum chromodynamics (QCD) and the phenomenon of color superconductivity.
Schaffner-Bielich, Jürgen
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Results from the STAR experiment
, 2002 Collisions of heavy ions at RHIC are expected to exceed the energy densities required to achieve a phase transition to the quark gluon plasma (QGP) [1,2].
STAR Collaboration +8 more
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Induced star formation in interacting galaxies
, 1987 Measurements of H alpha emission line fluxes and FIR fluxes in approx. 100 interacting spirals were used to investigate the effects of close tidal interactions on the disk and nuclear star formation rates in galaxies.
Vanderhulst, J. M. +4 more
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Bright transients from strongly-magnetized neutron star-black hole mergers [PDF]
, 2016 Direct detection of black hole-neutron star pairs is anticipated with the advent of aLIGO. Electromagnetic counterparts may be crucial for a confident gravitational-wave detection as well as for extraction of astronomical information.
Price, Larry +3 more
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