Results 101 to 110 of about 153,388 (301)

MORPHOLOGICAL TYPES OF 254 RICH PF GALAXY CLUSTERS

Odessa Astronomical Publications, 2014
We determined the morphological types for 254 rich galaxy clusters from the PF Catalogue of Galaxy Clusters and Groups. The data set contains the PF galaxy clusters, which have no ACO coinciding ones.
E. A. Panko, S. M. Andrievsky, A. V. Gotsulyak   +2 more
doaj   +1 more source

Galaxy Collisions, Gas Stripping and Star Formation in the Evolution of Galaxies

, 2004
A review of gravitational and hydrodynamical processes during formation of clusters and evolution of galaxies is given. Early, at the advent of N-body computer simulations, the importance of tidal fields in galaxy encounters has been recognized.
Palous, Jan
core   +1 more source

Stealing galaxies from galaxy clusters

Publications of the Astronomical Society of Australia
Abstract We investigate galaxy groups that reside in the field but have been previously processed by galaxy clusters. Observationally, they would appear to have the same properties as regular field groups at first glance. However, one would expect to find quantifiable differences in processed groups as dynamical interactions within clusters perturb ...
Majda Smole, Miroslav Micic, Ana Mitrašinović   +2 more
openaire   +2 more sources

Morphometric and External Injury Characterization of Rainbow Trout (O. mykiss) Used for Stocking in the Alpine River Inn (Bavaria, Germany)

Fisheries Management and Ecology, EarlyView.
ABSTRACT Stocking fish is a common practice in fisheries management, particularly for species of high conservation value or economic importance. Despite its widespread use, systematic evaluation of fish stockings remains scarce. This includes non‐native species such as rainbow trout (Oncorhynchus mykiss), which are intensively stocked into European ...
Christoffer Nagel, David Goldbrunner, Josef Knott, Joachim Pander, Juergen Geist   +4 more
wiley   +1 more source

COMPARISON OF OPTICAL AND X-RAY MASS ESTIMATES OF THE CHANDRA GALAXY CLUSTERS AT Z < 0.1

Odessa Astronomical Publications, 2013
We used the optical data taken from SDSS DR7 galaxy and group catalog to determine the optical mass of 37 nearer Chandra galaxy clusters for comparison with the X-ray mass estimates.
Iu. V. Babyk, I. B. Vavilova
doaj   +1 more source

The Sloan Great Wall. Rich clusters

, 2010
We present the results of the study of the substructure and galaxy content of ten rich clusters of galaxies in three different superclusters of the Sloan Great Wall.
Abazajian, Adelman-McCarthy, Aguerri, Anscombe, Ashman, Bamford, Bardelli, Barrena, Belsole, Berlind, Berrier, Biviano, Blake, Blanton, Blanton, Blanton, Boschin, Boschin, Bower, Burgett, Butcher, Böhringer, Coziol, Donnelly, Dressler, Dressler, D’Agostino, E. Saar, E. Tago, E. Tempel, Einasto, Einasto, Einasto, Einasto, Einasto, Einasto, Einasto, Einasto, Einasto, Eisenstein, Eisenstein, Fraley, Gott, Huchra, Huertas-Company, Hwang, Hwang, I. Enkvist, Ihaka, J. Einasto, J. Vennik, Knebe, Knollmann, Kofman, L. J. Liivamägi, Leisch, Ligges, Lintott, Loeb, M. Einasto, Malumuth, Martínez, Masters, Merritt, Mobasher, Nichol, Niemi, Oegerle, Oegerle, Ostriker, Ouchi, P. Einasto, P. Heinämäki, P. Nurmi, P. Pihajoki, Park, Park, Plionis, Ragone-Figueroa, Rose, Ruhland, Shapiro, Skelton, Solanes, Springel, Springel, Tago, Tempel, Tinker, Tovmassian, Turner, V. J. Martínez, Venemans, Vennik, Vogeley, Watson, Whitmore, Zehavi, Zeldovich, Zheng   +99 more
core   +1 more source

Epidemiology and Genetics of Rheumatic Diseases Suggest a Constant Rate of DNA Damage as Underlying Cause

Immunology, EarlyView.
A constant rate of DNA damage that is not perfectly repaired will cause a constant rate of DNA mutations. The chance of mutation will increase if DNA is prone to damage, such as occurs in somatic hypermutation (SHM) hotspots and GC‐rich DNA. Thus, if one mutation‐prone DNA site drives disease, the age of onset of disease and degree of penetrance should
Piet C. de Groen
wiley   +1 more source

Constraints on $\Omega_\mathrm{m}$ and $\sigma_8$ from the potential-based cluster temperature function

, 2015
The abundance of galaxy clusters is in principle a powerful tool to constrain cosmological parameters, especially $\Omega_\mathrm{m}$ and $\sigma_8$, due to the exponential dependence in the high-mass regime.
Angrick, Christian, Bartelmann, Matthias, Pace, Francesco, Roncarelli, Mauro   +3 more
core   +1 more source

Proteomic analysis of the zone of degeneration at the mitosis–meiosis transition stage in wild‐caught male catshark (Scyliorhinus canicula), correlated with an unusually high‐water temperature in the English Channel

Journal of Fish Biology, EarlyView.
Abstract In the context of current global change, variations in water temperature are one of the environmental conditions with serious consequences for marine life, including reproductive processes. In the small spotted catshark Scyliorhinus canicula, spermatogenesis occurs in spermatocysts composed of synchronously developing germ cells associated ...
Fabian Jeanne, Stanislas Pilet, Sean Heighton, Benoît Bernay, Pascal Sourdaine   +4 more
wiley   +1 more source

On the Particle Acceleration Mechanisms in a Double Radio Relic Galaxy Cluster, Abell 1240

The Astrophysical Journal
We present a 368 ks deep Chandra observation of Abell 1240, a binary merging galaxy cluster at a redshift of 0.195 with two brightest cluster galaxies that may have passed each other 0.3 Gyr ago.
Arnab Sarkar, Felipe Andrade-Santos, Reinout J. van Weeren, Ralph P. Kraft, Duy N. Hoang, Timothy W. Shimwell, Paul Nulsen, William Foreman, Scott Randall, Yuanyuan Su, Priyanka Chakraborty, Christine Jones, Eric Miller, Mark Bautz, Catherine E. Grant   +14 more
doaj   +1 more source