中文
相关论文

相关论文: Two Galaxy Clusters: A3565 and A3560

200 篇论文

We present a detailed study of the cluster CL 0048-2942, located at z~0.64, based on a photometric and spectroscopic catalogue of 54 galaxies in a 5 x 5 square arcmin region centred in that cluster. Of these, 23 galaxies were found to…

天体物理学 · 物理学 2009-11-10 M. Serote Roos , C. Lobo , F. Durret , A. Iovino , I. Marquez

We present Gemini optical spectroscopy of 23 young star clusters in NGC3256. We find that the cluster ages range are from few Myr to ~150 Myr. All these clusters are relatively massive (2--40)x 10^{5} \msun$ and appear to be of roughly 1.5…

天体物理学 · 物理学 2009-06-23 Gelys Trancho , Nate Bastian , Bryan W. Miller , François Schweizer

We present the results of a dynamical analysis of three rich, X-ray luminous galaxy clusters, Abell 222, Abell 223 and Abell 520, that are at intermediate redshifts. Our study is based on radial velocities for 71 cluster members,…

天体物理学 · 物理学 2007-05-23 D. Proust , H. Cuevas , H. V. Capelato , L. Sodre , B. Tome Lehodey , O. Le Fevre , A. Mazure , .

We present radial velocity and metallicity measurements for the far-southern Galactic globular cluster IC4499. We selected several hundred target red giant stars in and around the cluster from the 2MASS point source catalog, and obtained…

星系天体物理 · 物理学 2010-11-17 Warren J. Hankey , Andrew A. Cole

X-ray and radio observations of CIZA J2242.8+5301 suggest that it is a major cluster merger. Despite being well studied in the X-ray, and radio, little has been presented on the cluster structure and dynamics inferred from its galaxy…

We present images of the recent galaxy merger NGC 3256 obtained with the WFPC2 of the Hubble Space Telescope in B and I filters. We show that there is a large population of more than 1,000 compact, bright blue objects in this galaxy within…

天体物理学 · 物理学 2009-10-31 S. E. Zepf , K. M. Ashman , J. English , K. C. Freeman , R. M. Sharples

We report 2868 new multi-object spectroscopic measurements of galaxy redshifts in an area roughly 12\deg$\times$ 6\deg (right ascension $\times$ declination) centered on the Shapley Supercluster (SSC). These correspond to 2627 different…

天体物理学 · 物理学 2009-10-31 H. Quintana , Eleazar R. Carrasco , Andreas Reisenegger

We identify the extended Einstein IPC X-ray source, 1E0657-56, with a previously unknown cluster of galaxies at a redshift of $z=0.296$. Optical CCD images show the presence of a gravitational arc in this cluster and galaxy spectra yield a…

天体物理学 · 物理学 2016-08-30 W. Tucker , P. Blanco , S. Rappoport , L. David , D. Fabricant , E. E. Falco , W. Forman , A. Dressler , M. Ramella

Based on the DESI Legacy Imaging Surveys released data and available spectroscopic redshifts, we identify 1.58 million clusters of galaxies by searching for the overdensity of stellar mass distribution of galaxies within redshift slices…

宇宙学与河外天体物理 · 物理学 2024-04-03 Z. L. Wen , J. L. Han

We present an extensive spectroscopic follow-up campaign of 29 strong lensing (SL) selected galaxy clusters discovered primarily in the Second Red-Sequence Cluster Survey (RCS-2). Our spectroscopic analysis yields redshifts for 52…

Cosmological (LCDM) TreeSPH simulations of galaxy clusters have been performed, invoking star-formation, chemical evolution with non-instantaneous recycling, metal dependent radiative cooling, strong star-burst and/or AGN driven…

天体物理学 · 物理学 2009-11-10 J. Sommer-Larsen , A. D. Romeo , L. Portinari

We present a multi-wavelength study of RX J0848+4456, a cluster of galaxies discovered through X-ray emission in the ROSAT Deep Cluster Survey. Our observations consist of WFPC2 imaging, optical spectra, and X-ray data collected with the…

An extensive redshift survey has been conducted on a sample of 15 nearby (0.01 < z < 0.05) clusters of galaxies. A total number of 860 redshifts were determined by fitting of emission--lines and/or cross-correlation techniques. Of this…

天体物理学 · 物理学 2007-05-23 P. Stein

We present 1.4 and 2.5 GHz Australia Telescope Compact Array (ATCA) observations of the galaxy cluster A3158 (z=0.0597) which is located within the central part of the Horologium-Reticulum Supercluster (HRS). Spectroscopic data for the…

天体物理学 · 物理学 2009-11-13 M. Johnston-Hollitt , M. Sato , J. A. Gill , M. C. Fleenor , A. -M. Brick

As a part of our galaxy-cluster redshift survey, we present a set of 80 new velocities in the 4 clusters Abell 376, Abell 970, Abell 1356, and Abell 2244, obtained at Haute-Provence observatory. This set now completes our previous analysis,…

宇宙学与河外天体物理 · 物理学 2015-05-18 Dominique Proust , Hugo V. Capelato , Gastao B. Lima Neto , Laerte Sodre

Mass and concentration of clusters of galaxies are related and evolving with redshift. We study the properties of a sample of 31 massive galaxy clusters at high redshift, 0.8 < z < 1.5, using weak and strong lensing observations.…

宇宙学与河外天体物理 · 物理学 2015-06-16 Mauro Sereno , Giovanni Covone

We report optical imaging and spectroscopy of 41 galaxies in a 22 arcmin square region surrounding Cygnus A. The results show that there is an extensive rich cluster associated with Cygnus A of Abell richness at least 1 and possibly as high…

天体物理学 · 物理学 2009-10-30 Frazer N. Owen , Michael J. Ledlow , Glenn E. Morrison , John M. Hill

We present 118 new optical redshifts for galaxies in 12 clusters in the Horologium-Reticulum supercluster (HRS) of galaxies. For 76 galaxies, the data were obtained with the Dual Beam Spectrograph on the 2.3m telescope of the Australian…

We present a detailed dynamical analysis of the rich galaxy cluster A2744, containing a powerful diffuse radio halo.Our analysis is based on redshift data for 102 galaxies, part of them recovered from unexplored spectra in the ESO archive.…

天体物理学 · 物理学 2009-11-11 W. Boschin , M. Girardi , M. Spolaor , R. Barrena

AIMS: We present in this work low and intermediate resolution spectroscopic data collected for 152 early type galaxies in 8 nearby clusters with z $\leq$ 0.10. METHODS: We use low resolution data to produce the redshift and the K-correction…

天体物理学 · 物理学 2009-11-11 D. Bettoni , M. Moles , P. Kjaergaard , G. Fasano , J. Varela