Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR2.8k papers
- Heidelberg UniversityDE2.1k papers
- University of OxfordGB2k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR2k papers
- European Organization for Nuclear ResearchCH2k papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR2k papers
- Istituto Nazionale di Fisica Nucleare, Sezione di BolognaIT1.9k papers
- University of EdinburghGB1.9k papers
- The University of TokyoJP1.9k papers
- Ludwig-Maximilians-Universität MünchenDE1.9k papers
- University of ManchesterGB1.9k papers
- Institute of Nuclear Physics, Polish Academy of SciencesPL1.8k papers
7 papers · 2 filters
Dissipation of Magnetic Fields in the Galactic Halo
F. Zimmer, H. Lesch, G. T. Birk
This paper shows that magnetic reconnection could be an important heating process in cosmic gases. In any volume where magnetized plasmas collide, the dissipation of magnetic energ…
What perturbs NGC 2188?
H. Domgorgen, M. Dahlem, R. -J. Dettmar
VLA HI observations of the dwarf irregular galaxy NGC 2188 show that the gas and stars have spatial distributions which are substantially different. One end of the optical disk is…
Globular cluster systems of early--type galaxies in Fornax
M. Kissler-Patig, S. Kohle, M. Hilker +3
We studied the properties of the globular cluster systems of five early--type galaxies in the Fornax galaxy cluster: NGC 1374, NGC 1379, NGC 1387, NGC 1427, and the central giant e…
CIV absorption from hot gas inside supergiant shell LMC4 observed with HST and IUE
D. J. Bomans, K. S. de Boer, J. Koornneef +1
High resolution ultraviolet spectra with HST-GHRS of two stars in the direction of the supergiant shell LMC4 unambiguously show absorption by substantial quantities of CIV gas at v…
Molecular abundances in the Magellanic Clouds I. A multiline study of five cloud cores
Y. -N. Chin, C. Henkel, J. B. Whiteoak +3
Nine HII regions of the LMC were mapped in 13CO(1--0) and three in 12CO(1--0) to study the physical properties of the interstellar medium in the Magellanic Clouds. For N113 the mol…
The distance of the Fornax Cluster based on Globular Cluster Luminosity Functions
Sven Kohle, Markus Kissler-Patig, Michael Hilker +3
We present Globular Cluster Luminosity Functions for four ellipticals and one S0-Galaxy in the Fornax cluster of galaxies, derived from CCD photometry in V and I. The averaged turn…
Neutrino Trapping in a Supernova and Ion Screening
C. J. Horowitz
Neutrino-nucleus elastic scattering is reduced in dense matter because of correlations between ions. The static structure factor for a plasma of electrons and ions is calculated fr…