Outputs (264)

Resolving molecular gas in the central galaxies of cooling flow clusters (2003)
Journal Article
Edge, A., & Frayer, D. (2003). Resolving molecular gas in the central galaxies of cooling flow clusters. Astrophysical Journal Letters, 594(1), L13-L17. https://doi.org/10.1086/378386

We present aperture synthesis images of the CO (1-0) line emission in five central galaxies in cooling flow clusters using the Owens Valley Millimeter Array. Three of the five sources are significantly resolved, but the majority of the emission is fr... Read More about Resolving molecular gas in the central galaxies of cooling flow clusters.

The 2dF Galaxy Redshift Survey: galaxy clustering per spectral type (2003)
Journal Article
Madgwick, D., Hawkins, E., Lahav, O., Maddox, S., Norberg, P., Peacock, J., …Taylor, K. (2003). The 2dF Galaxy Redshift Survey: galaxy clustering per spectral type. Monthly Notices of the Royal Astronomical Society, 344(3), 847-856. https://doi.org/10.1046/j.1365-8711.2003.06861.x

We have calculated the two-point correlation functions in redshift space, ξ(σ, π), for galaxies of different spectral types in the 2dF Galaxy Redshift Survey. Using these correlation functions, we are able to estimate values of the linear redshift-sp... Read More about The 2dF Galaxy Redshift Survey: galaxy clustering per spectral type.

MEM03: The Second International Workshop on Mechano-Electromagnetic Properties of Composite Superconductors, Kyoto, Japan - Preface (2003)
Journal Article
Osamura, K., Wada, H., Nyilas, A., & Hampshire, D. (2003). MEM03: The Second International Workshop on Mechano-Electromagnetic Properties of Composite Superconductors, Kyoto, Japan - Preface. Superconductor Science and Technology, 16(9),

A scaling law for the critical current density of weakly- and strongly-coupled superconductors, used to parameterize data from a technological Nb3Sn strand (2003)
Journal Article
Keys, S., & Hampshire, D. (2003). A scaling law for the critical current density of weakly- and strongly-coupled superconductors, used to parameterize data from a technological Nb3Sn strand. Superconductor Science and Technology, 16(9), 1097-1108

Kinetics of the shear banding instability in startup flows (2003)
Journal Article
Fielding, S., & Olmsted, P. (2003). Kinetics of the shear banding instability in startup flows. Physical review E: Statistical physics, plasmas, fluids, and related interdisciplinary topics, 68(3), https://doi.org/10.1103/physreve.68.036313

Direct experimental evidence for the Ruderman-Kittel-Kasuya-Yosida interaction in rare-earth metals (2003)
Journal Article
Hindmarch, A., & Hickey, B. (2003). Direct experimental evidence for the Ruderman-Kittel-Kasuya-Yosida interaction in rare-earth metals. Physical Review Letters, 91(11), https://doi.org/10.1103/physrevlett.91.116601

The absorbing haloes around high-redshift radio galaxies: the UVES view (2003)
Journal Article
Wilman, R. J., Jarvis, M. J., Röttgering, H. J. A., & Binette, L. (2003). The absorbing haloes around high-redshift radio galaxies: the UVES view. New Astronomy Reviews, 47, 279-283. https://doi.org/10.1016/s1387-6473%2803%2900039-3

Proto-clusters and the clustering of distant galaxies and radio sources (2003)
Journal Article
Röttgering, H., Daddi, E., Overzier, R., & Wilman, R. (2003). Proto-clusters and the clustering of distant galaxies and radio sources. New Astronomy Reviews, 47, 309-314. https://doi.org/10.1016/s1387-6473%2803%2900129-5

X-ray emission properties of galaxies in Abell 3128 (2003)
Journal Article
Smith, R. J. (2003). X-ray emission properties of galaxies in Abell 3128. Monthly Notices of the Royal Astronomical Society, 344(2), L17–L21. https://doi.org/10.1046/j.1365-8711.2003.06963.x

The influence of grains on the propagation and structure of C-type shock waves in interstellar molecular clouds (2003)
Journal Article
Flower, D., & Pineau des Forêts, G. (2003). The influence of grains on the propagation and structure of C-type shock waves in interstellar molecular clouds. Monthly Notices of the Royal Astronomical Society, 343(2), 390-400. https://doi.org/10.1046/j.1365-8711.2003.06716.x

Gas–grain interactions can have important consequences for the physics and chemistry of shock waves propagating in molecular clouds. The grains can be both a source and a sink of molecules, and their inertia can modify the dynamics of the propagation... Read More about The influence of grains on the propagation and structure of C-type shock waves in interstellar molecular clouds.