Resonance Line Scattering Modifies X‐Ray Surface Brightness of Elliptical Galaxies
- 20 April 1998
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 497 (2) , 587-593
- https://doi.org/10.1086/305498
Abstract
No abstract availableThis publication has 9 references indexed in Scilit:
- X‐Ray Evidence for the Interaction of the Giant Elliptical Galaxy NGC 4472 with its Virgo Cluster EnvironmentThe Astrophysical Journal, 1996
- Discovery of a hierarchical distribution of dark matter in the Fornax cluster of galaxiesNature, 1996
- A ROSAT PSPC investigation of NGC 1399: cold gas and cooling flows in elliptical galaxiesMonthly Notices of the Royal Astronomical Society, 1995
- A fast operator perturbation method for the solution of the special relativistic equation of radiative transfer in spherical symmetryJournal of Quantitative Spectroscopy and Radiative Transfer, 1992
- The Astro-D missionAdvances In Space Research, 1990
- X-ray emission spectra from ionizing plasmasAstrophysics and Space Science, 1984
- The ROSAT missionAdvances In Space Research, 1982
- Soft X-ray spectrum of a hot plasmaThe Astrophysical Journal Supplement Series, 1977
- Hypernetted chain solutions for the classical one-component plasma up to Γ=7000The Journal of Chemical Physics, 1974