Results 31 to 40 of about 273,575 (267)

Ghostly Galaxies: Accretion-dominated Stellar Systems in Low-mass Dark Matter Halos

open access: yesThe Astrophysical Journal, 2023
Wide-area deep imaging surveys have discovered large numbers of extremely low surface brightness (LSB) dwarf galaxies, which challenge galaxy formation theory and, potentially, offer new constraints on the nature of dark matter.
Chung-Wen Wang   +4 more
doaj   +1 more source

The stellar halo metallicity—luminosity relationship for spiral galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society: Letters, 2005
Abstract The stellar haloes of spiral galaxies bear important chemodynamical signatures of galaxy formation. We present here the analysis of 89 semi-cosmological spiral galaxy simulations, spanning ∼4 mag in total galactic luminosity. These simulations sample a wide variety of merging histories and show significant dispersion in halo ...
Renda, Agostino   +6 more
openaire   +3 more sources

Stellar population gradients in galaxy discs from the CALIFA survey : the influence of bars [PDF]

open access: yes, 2014
We acknowledge financial support from the research projects under grants AYA2010-21887-C04-03, AYA2010-21322-C03-03 and AYA2010-15081 by the Spanish Ministerio de Ciencia e Innovación.While studies of gas-phase metallicity gradients in disc galaxies are ...
Wisotzki, L.   +73 more
core   +1 more source

Elliptical galaxies/stellar halos connection [PDF]

open access: yesProceedings of the International Astronomical Union, 2019
AbstractCosmological simulations predict that early-type galaxies (ETGs) are the results of extended mass accretion histories. The latter are characterized by different numbers of mergers, mergers’ mass ratios and gas fractions, and timing. Depending on the sequence and nature of these mergers that follow the first phase of the in-situ star formation ...
Arnaboldi, Magda   +3 more
openaire   +2 more sources

Galaxy And Mass Assembly (GAMA) : galaxy close pairs, mergers and the future fate of stellar mass [PDF]

open access: yes, 2014
ASGR acknowledges STFC and SUPA funding that were used to do this work. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO and the participating institutions.We use a highly complete subset of the Galaxy And Mass Assembly II (GAMA-II) redshift
De Propris, R.   +65 more
core   +1 more source

The Outer Halos of Very Massive Galaxies: BCGs and their DSC in the Magneticum Simulations

open access: yesGalaxies, 2017
Recent hydrodynamic cosmological simulations cover volumes up to Gpc 3 and resolve halos across a wide range of masses and environments, from massive galaxy clusters down to normal galaxies, while following a large variety of physical processes ...
Rhea-Silvia Remus   +2 more
doaj   +1 more source

Stellar Halos from the The Dragonfly Edge-on Galaxies Survey

open access: yesThe Astrophysical Journal, 2022
Abstract We present the primary results from the Dragonfly Edge-on Galaxies Survey, an exploration of the stellar halos of twelve nearby (d < 25 Mpc) edge-on disk galaxies with the Dragonfly Telephoto Array. The edge-on orientation of these galaxies allows their stellar halos to be explored with minimal obscuration by or confusion ...
Colleen Gilhuly   +8 more
openaire   +2 more sources

Kinematics and simulations of the stellar stream in the halo of the Umbrella Galaxy [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2014
23 pages, 10 figures, 7 tables, accepted for publication in MNRAS 3D animated gif N-body model: http://sages.ucolick.org/downloads/Umbrella_3d ...
Foster, C.   +11 more
openaire   +3 more sources

The progenitor galaxies of stellar haloes as ‘failed’ Milky Ways

open access: yesMonthly Notices of the Royal Astronomical Society, 2023
ABSTRACT The stellar halo of the Milky Way records the history of its interactions with dwarf galaxies, whose subsequent destruction results in the formation of an extended stellar component. Recent works have suggested that galaxies with masses comparable to the Large Magellanic Cloud (LMC, $M_\star \sim 10^9$ M☉) may be the primary ...
Sownak Bose, Alis J Deason
openaire   +3 more sources

From Halos to Galaxies. VII. The Connections between Stellar Mass Growth History, Quenching History, and Halo Assembly History for Central Galaxies

open access: yesThe Astrophysical Journal, 2023
The assembly of galaxies over cosmic time is tightly connected to the assembly of their host dark matter halos. We investigate the stellar mass growth history and the chemical enrichment history of central galaxies in the Sloan Digital Sky Survey Mapping
Cheqiu Lyu   +14 more
doaj   +1 more source

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