Results 41 to 50 of about 553,808 (287)

Magnetic fields in galaxies - I. Radio discs in local late-type galaxies [PDF]

Monthly Notices of the Royal Astronomical Society, 2010
10 pages, 8 figures; MNRAS in ...
Shabala, Stanislav, Mead, James M. G., Alexander, Paul   +2 more
openaire   +2 more sources

Morphological Distribution of Galaxies in Some Nearby Clusters

Open Astronomy, 2019
We study the morphological distribution of galaxies in some nearby clusters, using the Sloan Digital Sky Survey – Data Release 9 (SDSS-DR9). The segregation between early-type galaxies and late-type ones is investigated in g – r / u – g color space ...
Rasheed Mariwan A., Mohammad Khalid K.
doaj   +1 more source

The Classification of Galaxy Morphology in the H Band of the COSMOS-DASH Field: A Combination-based Machine-learning Clustering Model

The Astrophysical Journal Supplement Series, 2023
By applying our previously developed two-step scheme for galaxy morphology classification, we present a catalog of galaxy morphology for H -band-selected massive galaxies in the COSMOS-DASH field, which includes 17,292 galaxies with stellar mass M _ ...
Yao Dai, Jun Xu, Jie Song, Guanwen Fang, Chichun Zhou, Shuo Ba, Yizhou Gu, Zesen Lin, Xu Kong   +8 more
doaj   +1 more source

The dustier early-type galaxies deviate from late-type galaxies’ scaling relations [PDF]

Monthly Notices of the Royal Astronomical Society, 2016
MNRAS accepted; 12 pages, 9 figures, 5 ...
Lianou, S., Xilouris, E., Madden, S. C., Barmby, P.   +3 more
openaire   +4 more sources

The minor role of gas-rich major mergers in the rise of intermediate-mass early types at z <~ 1 [PDF]

, 2010
We study the evolution of galaxy structure since z ~ 1 to the present. From a GOODS-S multi-band catalog we define (blue) luminosity- and mass-weighted samples, limited by M_B = 10^10 M_Sun, comprising 1122 and 987 galaxies, respectively.
Adelman-McCarthy, Baldry, Bekki, Bell, Bell, Bell, Bershady, Bezanson, Blakeslee, Bridge, Buitrago, Bundy, Bundy, Bundy, Carlos López-Sanjuan, Cenarro, Combes, Conselice, Conselice, Conselice, Cristóbal-Hornillos, César Enrique García-Dabó, Dahlen, Davis, De Propris, de Vaucouleurs, Drory, Eliche-Moral, Faber, Fisher, Giavalisco, González-García, Guillermo Barro, Heiderman, Hopkins, Hopkins, Hopkins, Hopkins, Hopkins, Hopkins, Ilbert, Jaime Zamorano, Jesús Gallego, Jogee, Knapen, Kriek, Lauger, Lilly, Lin, Lin, Lotz, Lotz, López-Sanjuan, Marc Balcells, Marchesini, Martig, Menanteau, Naab, Naab, Oesch, Pablo G. Pérez-González, Papovich, Pérez-González, Pérez-González, Rawat, Rix, Robaina, Rothberg, Rothberg, Ruhland, Scarlata, Scarlata, Scoville, Somerville, Stewart, Strateva, Taylor, van der Wel, van der Wel, van der Wel, van Dokkum, Villar, Wolf, Zamojski   +83 more
core   +3 more sources

Age-density relation of Main galaxies at fixed parameters or for different galaxy families

Open Physics, 2015
Using two volume-limited Main galaxy samples of the Sloan Digital Sky Survey Data Release 10 (SDSS DR10), we examine the environmental dependence of galaxy age at fixed parameters or for different galaxy families.
Deng Xin-Fa, Song Jun, Chen Yi-Qing, Jiang Peng, Ding Ying-Ping   +4 more
doaj   +1 more source

The size distribution of galaxies in the Sloan Digital Sky Survey [PDF]

, 2003
abridged: We use a complete sample of about 140,000 galaxies from the Sloan Digital Sky Survey (SDSS) to study the size distribution of galaxies and its dependence on their luminosity, stellar mass, and morphological type.
Blanton, Michael R., Brinkmann, J., Csabai, Istvan, Kauffmann, Guinevere, Mo, H. J., Shen, Shiyin, Voges, Wolfgang, White, Simon D. M.   +7 more
core   +4 more sources

Intrinsic galaxy shapes and alignments I: Measuring and modelling COSMOS intrinsic galaxy ellipticities [PDF]

, 2013
The statistical properties of the ellipticities of galaxy images depend on how galaxies form and evolve, and therefore constrain models of galaxy morphology, which are key to the removal of the intrinsic alignment contamination of cosmological weak ...
Abraham, Allgood, Altay, B. Joachimi, Bailin, Bailin, Bartelmann, Bernstein, Bernstein, Bertin, Bett, Bett, Bett, Bildfell, Binggeli, Binney, Bower, Brainerd, Bridle, Bridle, Bundy, Catelan, Cole, Croft, Davis, E. Semboloni, Erben, Faltenbacher, Fukugita, H. Hoekstra, Hahn, Hahn, Hao, Harker, Heavens, Heymans, Heymans, Hilbert, Hirata, Hoekstra, Hung, Ilbert, J. Hartlap, Jing, Joachimi, Joachimi, Joachimi, Joachimi, Kaiser, Kazantzidis, King, King, Kitching, Knebe, Knebe, Komatsu, Kuhlen, Lambas, Laureijs, Leauthaud, Lee, Mandelbaum, Mandelbaum, Melchior, Mobasher, P. E. Bett, P. Schneider, Parry, Percival, Pereira, Refregier, Rhodes, S. Hilbert, Scarlata, Schneider, Schrabback, Scoville, Spergel, Springel, Springel, T. Schrabback, Takada, van den, van Uitert, Zhang   +84 more
core   +2 more sources

Galaxy morphology classification: are stellar circularities enough? [PDF]

Serbian Astronomical Journal
We present a preliminary study exploring whether the stellar orbital circularity of simulated galaxies, available from precomputed catalogs in the IllustrisTNG project, can be used as a proxy for a broad morphological classification. We focus on
Baucalo Katarina, Mitrašinović Ana
doaj   +1 more source

The population of early-type galaxies: how it evolves with time and how it differs from passive and late-type galaxies [PDF]

, 2014
The aim of our analysis is twofold. On the one hand we are interested in addressing whether a sample of ETGs morphologically selected differs from a sample of passive galaxies in terms of galaxy statistics.
S. Tamburri, P. Saracco, M. Longhetti, A. Gargiulo, I. Lonoce, F. Ciocca   +5 more
semanticscholar   +1 more source