Results 51 to 60 of about 211,606 (245)
Morphological Evolution of Galaxies [PDF]
29 pages (AAS latex) + 7 figures (postscript) combined in one gzip-ed tar file. Submitted to The Astrophysical Journal (Dec 1996)
Hugo Martel +4 more
openaire +4 more sources
Stellar populations in gas-rich galaxy mergers I. Dependence on star formation history
We investigate the nature of stellar populations of major galaxy mergers between late-type spirals considerably abundant in interstellar medium by performing numerical simulations designed to solve both the dynamical and chemical evolution in a self ...
Bekki, Kenji, Shioya, Yasuhiro
core +1 more source
With Gaia, APOGEE, GALAH, and LAMOST data, we investigate the positional, kinematic, chemical, and age properties of nine moving groups in the solar neighborhood.
Xilong Liang, Suk-Jin Yoon, Jingkun Zhao
doaj +1 more source
Bar Formation in Milky Way type Galaxies
Many barred galaxies, possibly including the Milky Way, have cusps in their centers. There is a widespread belief, however, that the usual bar instability, which occurs in bulgeless galaxy models, is impossible for cuspy models because of the presence of
Polyachenko E. V., Berczik P., Just A.
doaj +1 more source
Cosmological evolution of galaxies [PDF]
I review the subject of the cosmological evolution of galaxies, including different aspects of growth in disk galaxies, by focussing on the angular momentum problem, mergers, and their by-products. I discuss the alternative to merger-driven growth -- cold accretion and related issues.
openaire +3 more sources
We present the most accurate measurement to date of cosmological evolution of the near-infrared galaxy luminosity function, from the local Universe out to z~4.
Bershady +99 more
core +1 more source
We present an empirical chemical evolution model that explains the distribution of metals in the interstellar medium (ISM) and the circumgalactic medium (CGM) of galaxies based on the U niverse M achine and N eutral U niverse M achine models in the ...
Moka Nishigaki +7 more
doaj +1 more source
Arp 220: A Post-starburst Galaxy with Little Current Star Formation outside of Its Nuclear Disks
The ultraluminous infrared galaxy Arp 220 is a late-stage merger with several tidal structures in the outskirts and two very compact, dusty nuclei that show evidence for extreme star formation and host at least one active galactic nucleus (AGN).
Rupali Chandar +10 more
doaj +1 more source
Evolution of galaxy habitability [PDF]
We combine a semi-analytic model of galaxy evolution with constraints on circumstellar habitable zones and the distribution of terrestrial planets to probe the suitability of galaxies of different mass and type to host habitable planets, and how it evolves with time.
Sungwook E. Hong, Raphael Gobat
openaire +4 more sources
Galaxy formation with radiative and chemical feedback [PDF]
Here we introduce GAMESH, a novel pipeline which implements self-consistent radiative and chemical feedback in a computational model of galaxy formation. By combining the cosmological chemical-evolution model GAMETE with the radiative transfer code CRASH,
de Bennassuti, M. +5 more
core +3 more sources

