Results 1 to 10 of about 5,855,247 (377)

Dwarf Galaxy Formation Induced by Galaxy Interactions [PDF]

The Astrophysical Journal, 2000
9 pages (including 1 figure), To appear in ApJ, 543 (Part 1) Nov 1, 2000 (ApJ volume Nr was wrong in the previous version ...
Tadashi Okazaki, Yoshiaki Taniguchi
semanticscholar   +7 more sources

Active galactic nuclei and galaxy interactions [PDF]

Monthly Notices of the Royal Astronomical Society, 2007
We perform a statistical analysis of AGN host characteristics and nuclear activity for AGNs in pairs and without companions. Our study concerns a sample of AGNs derived from the SDSS-DR4 data by Kauffmann et al (2003) and pair galaxies obtained from the same data set by Alonso et al. (2006).
M. S. Alonso, D. G. Lambas, P. B. Tissera, Georgina Coldwell   +3 more
semanticscholar   +8 more sources

Combined Effects of Galaxy Interactions and Large-Scale Environment on Galaxy Properties [PDF]

, 2008
We inspect the coupled dependence of physical parameters of the SDSS galaxies on the small-scale (distance to and morphology of the nearest neighbor galaxy) and the large-scale (background density smoothed over 20 nearby galaxies) environments.
Adelman-McCarthy, Allam, Balogh, Barnes, Barton, Barton, Barton, Bell, Binney, Blanton, Blanton, Blanton, Blanton, Brighenti, Brown, Brown, Changbom Park, Choi, Conroy, Coziol, D'Onghia, de Propris, Ellison, Evrard, Geller, Gomez, Gott, Graham, Henriksen, Hernandez-Toledo, Hogg, Jeltema, Kacprzak, Kim, Li, Maller, Matsushita, Mendes de Oliveira, Naab, Park, Park, Park, Park, Patton, Patton, Poggianti, Prada, Quintero, Robertson, Schlegel, Smith, Tanaka, Tegmark, Tran, Tully, Ulmer, van den Bergh, van der Wel, van Dokkum, Woods, Woods, Yang, York, Yun-Young Choi   +63 more
core   +3 more sources

Interaction of Galaxies with the ICM

, 2003
In recent years a wealth of data and detailed hydrodynamical simulations have appeared that show the effects of interactions between the ICM and galaxies. Single dish observations show that cluster galaxies are deficient in their HI content out to 2 Abell radii. The deficient galaxies tend to be on radial orbits.
J. H. van Gorkom
openalex   +4 more sources

The SEDs of interacting galaxies [PDF]

Proceedings of the International Astronomical Union, 2011
AbstractThe evolution of galaxies is greatly influenced by their interactions. As part of a program to study interacting galaxies, we have measured and modeled the spectral energy distributions (SEDs) from the ultraviolet (UV) to the far-infrared (FIR).
Elisabete da Cunha, C. R. Klein, Matthew L. N. Ashby, Christopher C. Hayward, Lauranne Lanz, Patrik Jonsson, Giovanni G. Fazio, Nicola Brassington, Howard A. Smith, Lars Hernquist, Andreas Zezas   +10 more
openaire   +4 more sources

INTERACTIONS OF GALAXIES IN THE GALAXY CLUSTER ENVIRONMENT [PDF]

The Astrophysical Journal, 2009
We study the dependence of galaxy properties on the clustercentric radius and the environment attributed to the nearest neighbor galaxy using the SDSS galaxies associated with the Abell galaxy clusters. We find that there exists a characteristic scale where the properties of galaxies suddenly start to depend on the clustercentric radius at fixed ...
Changbom Park, Ho Seong Hwang
openaire   +3 more sources

H i 21 cm Extended Structures to the Northeast and Southwest of NGC 5595: VLA Observations of the Disk Galaxy Pair NGC 5595 and NGC 5597

The Astronomical Journal, 2023
We report VLA B-configuration observations of the H i 21 cm line on the close disk galaxy pair NGC 5595 and NGC 5597. At the angular resolution of the observations, ∼7.″1 × 4.″2, while most of the H i 21 cm in NGC 5595 and NGC 5597 has the same extent as
J. Antonio Garcia-Barreto, Emmanuel Momjian   +1 more
doaj   +1 more source

Triggering Star Formation by Galaxy-Galaxy Interactions [PDF]

Symposium - International Astronomical Union, 2004
We analyzed the effects of having a close companion on the star formation activity of galaxies in the 8K galaxy pair catalog selected from the 2dFGRS. We found that, statistically, galaxies with rp < 25h−1 kpc and ΔV < 100km s−1 have enhanced star formation with respect to isolated galaxies with the same luminosity and redshift distribution.
M. S. Alonso, Diego G. Lambas, P. B. Tissera, G. Coldwell   +3 more
openaire   +3 more sources

THE METALLICITY EVOLUTION OF INTERACTING GALAXIES [PDF]

The Astrophysical Journal, 2012
Nuclear inflows of metal-poor interstellar gas triggered by galaxy interactions can account for the systematically lower central oxygen abundances observed in local interacting galaxies. Here, we investigate the metallicity evolution of a large set of simulations of colliding galaxies.
Torrey, Paul, Cox, T J, Kewley, Lisa, Hernquist, Lars   +3 more
openaire   +4 more sources

Interacting galaxies and cosmological parameters [PDF]

Astronomy & Astrophysics, 2006
We propose a (physical)-geometrical method to measure the present rates of the density cosmological parameters for a Friedmann-Lemaitre universe. The distribution of linear separations between two interacting galaxies,when both of them undergo a first massive starburst, is used as a standard of length.
Reboul, Henri, Cordoni, J.-P.
openaire   +4 more sources