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Topic: Catalogue of Galaxies and of Clusters of Galaxies


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  Bill Keel's Publication List
The Stellar Population in the Wolf-Rayet Knot in NGC 5430, Astron.
Galaxy Cluster Formation from the Large-Scale Structure: A Case Study of the Abell 2125 Complex at z=0.247, Q. Daniel Wang, Frazer Owen, Michael Ledlow, and William Keel, in Outskirts of Galaxy Clusters: Intense Life in the Suburbs, IAU Coll.
Escape of Lyman alpha from the ISM in the starburst galaxy Mkn 357, W.C. Keel, BAAS 33, 1373 (49.06), 2001.
www.astr.ua.edu /keel/publist.html   (5542 words)

  
 Globular Star Clusters
Globular clusters typically contain a number of variable stars, in particular RR Lyrae stars which were once called "Cluster Variables" because of their abundance in globulars.
It is perhaps a bit surprising that almost all globular clusters seem to be of about the same age; there seems to be a physical reason that they all formed in a short period of time in the history of the universe, and this period was apparently long ago when the galaxies were young.
These galaxies contain also extremely large diffuse nebulae with masses of the order of globular clusters, clear candidates for future young globulars currently in formation, notably the Tarantula Nebula NGC 2070 in the LMC and NGC 604 in M33.
www.seds.org /messier/glob.html   (2112 words)

  
 Bibliography
A Catalog of Elliptical Galaxies with Shells (With D. Carter) Ap J. While the discovery of shells around elliptical galaxies was unexpected, the generality of the phenomenon was very surprising.
A comparison of the detection of faint images of clusters of galaxies using the eye and automatic measuring machines on photographically amplified images.
Catalogue of the Universe by Paul Murdin, David Allen and David Malin.
www.aao.gov.au /images/general/bibliography.html   (2869 words)

  
 PUBLICATIONS:
M. Pierre, and J.L. Starck, "X-ray structures in galaxy cores", Astronomy and Astrophysics, 330, 3, 801--818, 1998.
J.L. Starck, P. Querre, and V.J. Martinez, "Analysis of the galaxy distribution using multiscale methods", in SPIE Conference on Astronomical Data Analysis Conference, J.L. Starck and F. Murtagh Eds, Vol 4847, 2002.
D.L. Donoho and O. Levi and J.-L. Starck and V.J. Martinez, "Multiscale Geometric Analysis for 3-D Catalogues", in SPIE Conference on Astronomical Data Analysis Conference, J.L. Starck and F. Murtagh Eds, Vol 4847, 2002.
jstarck.free.fr /publi.htm   (5758 words)

  
 Giuseppe Tanzella-Nitti Personal Home Page
Palumbo, G., Tanzella-Nitti, G., Vettolani, G., Description of a Catalogue of Radial Velocities of Galaxies, in «Clustering in the Universe», Gerbal and Mazure Eds., Editions Fronteries, Paris 1983, pp.
Palumbo, G., Vettolani, G., Tanzella-Nitti, G., The Catalogue of Radial Velocities of Galaxies (abstract), in Proceedings of the I.A.U Colloquium «Early Evolution of the Universe and its Present Structure», Abell and Chincarini Eds., Reidel, Dordrecht 1984, p.
Tanzella-Nitti, G., Radial velocities of Galaxies: some considerations on the the comparison between radio and optical data, in «Astronomy and Astrophysics Suppl.
www.disf.org /tanzella-nitti/pubblicazioni.htm   (287 words)

  
 Brown Library Resources: Astronomy Research Guide
Infrared detector technology has made such huge advances in the past decade that the only existing near-infrared sky survey, which was carried out at Caltech nearly 25 years ago, no longer serves as a useful context within which to interpret observations or select sources for study.
The University of Massachusetts is therefore leading a new project, called the Two Micron All Sky Survey (2MASS), which will canvas the entire sky for stars and galaxies as much as 50,000 times fainter than the stars seen in the last survey.
The National Space Science Data Center (NSSDC) archives and provides access to a wide variety of astrophysics, space physics, solar physics, lunar and planetary data from NASA space flight missions, in addition to selected other data and some models and software.
www.lib.virginia.edu /science/guides/s-astr.htm   (1234 words)

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