Results 91 to 100 of about 150,051 (304)

On the Internal Absorption of Galaxy Clusters

, 2000
A study of the cores of galaxy clusters with the Einstein SSS indicated the presence of absorbing material corresponding to 1E+12 Msun of cold cluster gas, possibly resulting from cooling flows.
Allen S. W., Allen S. W., Arnaud M., Braine J., Braine J., Briel U. G., Crovisier J., Daines S. J., Edge A. C., Fabian A. C., Ferland G. J., Fukazawa Y., Hansen L., Jaffe W., Jaffe W., Jaffe W., Jaffe W., Joel N. Bregman, John S. Arabadjis, Matsumomo H., McNamara B. R., Mewe R., Mewe R., Norgaard-Nielsen H. U., O’Dea C. P., Siddiqui H., Tsai J. C., White D. A., White D. A.   +28 more
core   +2 more sources

Constraints on Nonthermal Pressure at Galaxy Cluster Outskirts from a Joint SPT and XMM-Newton Analysis

The Astrophysical Journal Letters
We present joint South Pole Telescope and XMM-Newton observations of eight massive galaxy clusters (0.8–2 × 10 ^15 M _⊙ ) spanning a redshift range of 0.16–0.35. Employing a novel Sunyaev–Zel’dovich + X-ray fitting technique, we effectively constrain the
Arnab Sarkar, Michael McDonald, Lindsey Bleem, Mark Bautz, Bradford A. Benson, Priyanka Chakraborty, Catherine E. Grant, Christine Jones, Florian Kéruzoré, Eric D. Miller, Scott Randall, Charles Romero, Taweewat Somboonpanyakul, Yuanyuan Su   +13 more
doaj   +1 more source

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

Galaxy Clusters Selected via the Sunyaev–Zel'dovich Effect in the SPTpol 100-square-degree Survey [PDF]

, 2020
We present a catalog of galaxy cluster candidates detected in 100 square degrees surveyed with the SPTpol receiver on the South Pole Telescope. The catalog contains 89 candidates detected with a signal-to-noise ratio greater than 4.6.
Crites, A. T., Huang, N., Moran, C. Corbett, Padin, S.   +3 more
core  

ATAC‐seq in Emerging Model Organisms: Challenges and Strategies

Journal of Experimental Zoology Part B: Molecular and Developmental Evolution, EarlyView.
Principle of ATAC‐seq (left), overview of arthropod species with published ATAC‐seq data (middle), summary of experimental design (right). ABSTRACT The Assay for Transposase‐Accessible Chromatin with sequencing (ATAC‐seq) is a versatile and widely utilized method for identifying potential regulatory regions, such as promoters and enhancers, within a ...
Duğçar Ebrar Erdoğan, Shadi Karimifard, Mozhgan Khodadadi, Liucong Ling, Luisa Linke, Ana Catalán, Vincent Doublet, Amanda Glaser‐Schmitt, Oliver Niehuis, Katja Nowick, Antonella Soro, Natascha Turetzek, Barbara Feldmeyer, Nico Posnien   +13 more
wiley   +1 more source

Low Injection Rate of Cosmic-Ray Protons in the Turbulent Reacceleration Model of Radio Halos in Galaxy Clusters

The Astrophysical Journal
A giant radio halo (RH) is a diffuse synchrotron emission observed on the scale of megaparsecs, typically found in the central region of merging galaxy clusters.
Kosuke Nishiwaki, Katsuaki Asano
doaj   +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

Somato‐Cognitive Action Network in Focal Dystonia

Movement Disorders, EarlyView.
Abstract Background The central pathology causing idiopathic focal dystonia remains unclear. The recently identified somato‐cognitive action network (SCAN) has been implicated. Objective We tested whether the effector‐agnostic SCAN may constitute a central pathology shared across dystonia subtypes, whereas the effector‐specific regions in the primary ...
Yuchao Wang, Baothy Huynh, Jianxun Ren, Mo Chen, Wei Zhang, Dan Hu, Shasha Li, Hesheng Liu, Teresa J. Kimberley   +8 more
wiley   +1 more source