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相关论文: Possible Connexion Between Large Scale Structures

200 篇论文

What is the role of clusters of galaxies in probing the large-scale velocity field of the universe? We investigate the distribution of peculiar velocities of clusters of galaxies in the popular low-density ($\Omega=0.3$) flat…

天体物理学 · 物理学 2009-10-22 Neta A. Bahcall , Renyue Cen , Mirt Gramann

An update of the evidence that radio galaxies and clusters of galaxies are more common than average near the plane of the de Vaucouleurs Local Supercluster shows that in the distance range 100 to 200Mpc objects whose positions are…

星系天体物理 · 物理学 2026-05-13 P. J. E. Peebles

Connecting galaxies with their descendants (or progenitors) at different redshifts can yield strong constraints on galaxy evolution. Observational studies have historically selected samples of galaxies using a physical quantity, such as…

星系天体物理 · 物理学 2015-05-20 Carl J. Mundy , Christopher J. Conselice , Jamie R. Ownsworth

We analyse the distribution of position angles of 1 million galaxies from the Hyperleda catalogue, a sample that presents the galaxies coordinates in the celestial sphere, information that allows us to look for a possible privileged…

宇宙学与河外天体物理 · 物理学 2017-05-08 R. S. Menezes , C. Pigozzo , S. Carneiro

We measure the projected half-light radii of young star clusters in 31 galaxies from the Legacy Extragalactic UV Survey (LEGUS). We implement a custom pipeline specifically designed to be robust against contamination, which allows us to…

星系天体物理 · 物理学 2021-10-20 Gillen Brown , Oleg Y. Gnedin

Clusters of galaxies are merging during the formation of large-scale structures in the Universe. Based on optical survey data, we identify a large sample of pre-mergers of galaxy clusters and merging subclusters in rich clusters. We find…

宇宙学与河外天体物理 · 物理学 2024-06-04 Z. L. Wen , J. L. Han , Z. S. Yuan

The distribution of nearby (cz < 7500 km/s) galaxies has been explored by minimal spanning trees; allowance has been made for the drastic decrease of data with distance. The investigation finds that all galaxies are members of irregular…

天体物理学 · 物理学 2007-05-23 Anthony Fairall , D. Turner , M. L. Pretorius , M. Wiehahn , V. McBride , G. de Vaux , P. A. Woudt

We used the Revised Flat Galaxy Catalog (RFGC) to select 817 ultra-flat (UF) edge-on disk galaxies with blue and red apparent axial ratios of $(a/b)_B > 10.0$ and $(a/b)_R > 8.5$. The sample covering the whole sky, except the Milky Way…

星系天体物理 · 物理学 2016-06-01 I. D. Karachentsev , V. E. Karachentseva , Yu. N. Kudrya

(abridged) We present the results of a redshift survey of intercluster galaxies in the central region of the Shapley Concentration supercluster, aimed at determining the distribution of galaxies in between obvious overdensities. Our sample…

天体物理学 · 物理学 2009-10-31 S. Bardelli , E. Zucca , G. Zamorani , L. Moscardini , R. Scaramella

A magnitude limited sample of nearly 9000 early-type galaxies, in the redshift range 0.01 < z < 0.3, was selected from the Sloan Digital Sky Survey using morphological and spectral criteria. The sample was used to study how early-type…

We analyze a sample of 23 supermassive elliptical galaxies (central velocity dispersion larger than 330 km s-1), drawn from the SDSS. For each object, we estimate the dynamical mass from the light profile and central velocity dispersion,…

宇宙学与河外天体物理 · 物理学 2015-05-20 O. Tiret , P. Salucci , M. Bernardi , C. Maraston , J. Pforr

We have conducted a galaxy survey based on low-resolution slitless spectra taken from the automated CFHT-Laval survey. We present redshift distributions for 522 galaxies distributed in 4 distinct regions of the sky. Redshifts are determined…

天体物理学 · 物理学 2015-06-24 M. Beauchemin , E. F. Borra

We have visually examined twelve Palomar red Plates for galaxies at low Galactic latitude b, where the Supergalactic Plane (SGP) is crossed by the Galactic Plane (GP), at Galactic longitude l ~135 degrees. The catalogue consists of 2575…

天体物理学 · 物理学 2015-06-24 G. K. T. Hau , H. C. Ferguson , O. Lahav , D. Lynden-Bell

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 a catalogue of 16551 edge-on galaxies created using the public DR2 data of the Pan-STARRS survey. The catalogue covers the three quarters of the sky above Dec.=-30 degrees. The galaxies were selected using a convolutional neural…

This is the first of a series of papers devoted to the investigation of a large sample of brightest cluster galaxies (BCGs), their kinematic and stellar population properties, and the relationships between those and the properties of the…

天体物理学 · 物理学 2009-11-13 S. I. Loubser , A. E. Sansom , P. Sanchez-Blazquez , I. K. Soechting , G. E. Bromage

We cross-matched the 4XMM-DR10 catalog with the HyperLEDA database and obtained the new sample of galaxies that contain X-ray sources. Excluding duplicate observations and false matches, we present a total of 7759 galaxies with X-ray…

星系天体物理 · 物理学 2023-02-08 N. Pulatova , A. Tugay , L. Zadorozhna , R. Seeburger , O. Gugnin

We present the catalog of galaxy groups in the Local Supercluster. Our algorithm bases on assumption that a total energy of physical pair of galaxies must be negative. About 54% of the galaxies in our sample have been gathered in 1082…

宇宙学与河外天体物理 · 物理学 2015-05-13 D. Makarov , I. Karachentsev

We present the largest publicly available catalogue of compact groups of galaxies identified using the original selection criteria of Hickson, selected from the Sixth Data Release (DR6) of the Sloan Digital Sky Survey (SDSS). We identify…

天体物理学 · 物理学 2009-11-13 Alan McConnachie , David Patton , Sara Ellison , Luc Simard

An updated catalogue of 76 galaxies with direct supermassive black hole mass measurements (M_bh) plus, when available, their host bulge's central velocity dispersion (sigma_0) is provided. Fifty of these mass measurements are considered…

天体物理学 · 物理学 2012-04-26 Alister W. Graham