The extended H -emitting filaments surrounding NGC 4696, the central galaxy of the Centaurus cluster
- 11 October 2005
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 363 (1) , 216-222
- https://doi.org/10.1111/j.1365-2966.2005.09463.x
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This publication has 27 references indexed in Scilit:
- Adaptive spatial binning of integral-field spectroscopic data using Voronoi tessellationsMonthly Notices of the Royal Astronomical Society, 2003
- On the Nature of the NGC 1275 SystemThe Astronomical Journal, 2001
- Evolution of Buoyant Bubbles in M87The Astrophysical Journal, 2001
- ASCA and ROSAT observations of nearby cluster cooling flowsMonthly Notices of the Royal Astronomical Society, 2001
- The ROSAT Brightest Cluster Sample -- III. Optical spectra of the central cluster galaxiesMonthly Notices of the Royal Astronomical Society, 1999
- The interaction of the radio halo of M87 with the cooling intracluster medium of the Virgo clusterMonthly Notices of the Royal Astronomical Society, 1995
- Photoelectric absorption cross sections with variable abundancesThe Astrophysical Journal, 1992
- Reddening estimates for galaxies in the Second Reference Catalog and the Uppsala General CatalogThe Astrophysical Journal Supplement Series, 1984
- Parameter estimation in astronomy through application of the likelihood ratioThe Astrophysical Journal, 1979
- A survey of interstellar H I from L-alpha absorption measurements. IIThe Astrophysical Journal, 1978