Results 31 to 40 of about 6,993,200 (327)

Galaxy workflow from Galaxy 101 for everyone

, 2021
Galaxy workflow from Galaxy 101 for everyone. This workflow is used in the training "How to reproduce published Galaxy analyses" to learn how to run a published Galaxy ...
Melanie Föll, Anne Fouilloux
core   +1 more source

Integral field spectroscopy with SINFONI of VVDS galaxies I. Galaxy dynamics and mass assembly at 1.2 < z < 1.6 [PDF]

, 2009
Context. Identifying the main processes of galaxy assembly at high redshifts is still a major issue in understanding galaxy formation and evolution at early epochs in the history of the Universe. Aims.
J. Queyrel, T. Contini, E. Pérez-Montero, B. Garilli, O. Le Fèvre, M. Kissler-Patig, B. Epinat, D. Vergani, L. Tresse, P. Amram, M. Lemoine-Busserolle   +10 more
semanticscholar   +1 more source

The Dynamics of Radio Galaxies and Double–Double Radio Galaxies [PDF]

Journal of Astrophysics and Astronomy, 2011
11 pages, 4 figures, Diffuse Radio Plasma Conference proceedings (held in Raman Research Institute, Bangalore, India)
Konar, C., Jamrozy, Marek, Hardcastle, M. J., Croston, J. H., Nandi, S., Saikia, D. J., Machalski, Jerzy   +6 more
openaire   +3 more sources

Cluster galaxy dynamics and the effects of large-scale environment [PDF]

, 2010
Advances in observational capabilities have ushered in a new era of multi-wavelength, multi-physics probes of galaxy clusters and ambitious surveys are compiling large samples of cluster candidates selected in different ways.
M. White, J. Cohn, R. Smit
semanticscholar   +1 more source

Galaxy Zoo: Mergers – Dynamical models of interacting galaxies [PDF]

Monthly Notices of the Royal Astronomical Society, 2016
The dynamical history of most merging galaxies is not well understood. Correlations between galaxy interaction and star formation have been found in previous studies, but require the context of the physical history of merging systems for full insight into the processes that lead to enhanced star formation.
Holincheck, A, Wallin, J, Borne, K, Fortson, L, Lintott, C, Smith, A, Bamford, S, Keel, W, Parrish, M   +8 more
openaire   +4 more sources

No need for dark matter: resolved kinematics of the ultra-diffuse galaxy AGC 114905 [PDF]

, 2021
We present new H i interferometric observations of the gas-rich ultra-diffuse galaxy AGC 114905, which previous work, based on low-resolution data, identified as an outlier of the baryonic Tully-Fisher relation.
P. M. Mancera Piña, F. Fraternali, T. Oosterloo, E. Adams, K. Oman, L. Leisman   +5 more
semanticscholar   +1 more source

Galaxy And Mass Assembly (GAMA) : the galaxy luminosity function within the cosmic web [PDF]

, 2015
EE acknowledges support from the Science and Technology Facilities Council. TMR acknowledges support from a ERC Starting Grant (DEGAS-259586). CH acknowledges support from the ERC under the EC FP7 grant number 240185.
Loveday, J, Baldry, I., E Eardley (16219808), T McNaught-Roberts (16161611), Driver, S. P., M E Cluver (16161572), M Alpaslan (16114469), I Baldry (16191140), Robotham, ASG, Robotham, A., Liske, J, Jonathan Loveday (4460899), Norberg, P, Driver, S.P., Eardley, E, Brough, S ; https://orcid.org/, Alpaslan, M., J Bland-Hawthorn (16111139), D J Farrow (16219811), Farrow, DJ, A S G Robotham (16143614), McNaught-Roberts, T., Brough, S., Loveday, J., Driver, SP, Liske, J., Farrow, D., Heymans, C, P Norberg (16143575), Peacock, JA, Alpaslan, M, J A Peacock (16045217), Robotham, A. S. G., Heymans, C., Bland-Hawthorn, J., Farrow, D. J., Bland-Hawthorn, J, Robotham, A.S.G., Baldry, I, Farrow, D.J., Peacock, J. A., Cluver, M., Driver, S., S Brough (16143590), McNaught-Roberts, T, Peacock, J.A., Norberg, P., J Liske (7814738), Eardley, E., Cluver, ME, Peacock, J., Cluver, M.E., C Heymans (16161599), Cluver, M. E., S P Driver (16143581)   +54 more
core   +1 more source

A dynamical model of the inner Galaxy [PDF]

Monthly Notices of the Royal Astronomical Society, 2000
20 pages, 5 gif figures, 11 postscript figures, submitted to MNRAS.
Hafner, R, Evans, NW, Dehnen, W, Binney, J   +3 more
openaire   +3 more sources

Elliptical Galaxy Dynamics [PDF]

, 1998
,(a b)/a with a and b the major- and minor-axis lengths. Hubble understood that the observed ellipticity was only a lower limit to the true elongation because of the unknown orientation of a galaxy’s “polar axis”; he called this uncertainty “serious, but
D. Merritt
semanticscholar   +1 more source

Galaxy Dynamics: Secular Evolution and Accretion [PDF]

Proceedings of the International Astronomical Union, 2010
Recent results are reviewed on galaxy dynamics, bar evolution, destruction and re-formation, cold gas accretion, gas radial flows and AGN fueling, minor mergers. Some problems of galaxy evolution are discussed in particular, exchange of angular momentum,
F. Combes
semanticscholar   +1 more source