Results 121 to 130 of about 37,027 (256)
What Does the LMC Look Like? It Depends on [M/H] and Age
We offer a new way to look at the LMC through stellar mono-abundance and mono-age mono-abundance maps. These maps are based on ≳500,000 member stars with estimates of [M/H] ( σ _[M/H] ~ 0.17) and age $({\sigma }_{{\rm{log}}\tau }\unicode{x0007E}0.15$ ),
Neige Frankel +4 more
doaj +1 more source
Erratum: Surface Photometry of Low Surface Brightness Dwarf Irregular Galaxies [PDF]
Richard J. Patterson, T. X. Thuan
openalex +1 more source
Discovery of Metal-poor and Distant Pre–Main Sequence Candidates in WLM with JWST
We present the discovery of 12 metal-poor and distant pre–main sequence (PMS) candidates in the dwarf irregular galaxy Wolf–Lundmark–Melotte ∼968 kpc away, at a present-day metallicity of [Fe/H] ∼ –0.9.
Venu M. Kalari +6 more
doaj +1 more source
LBT/MODS spectroscopy of globular clusters in the irregular galaxy NGC 4449 [PDF]
F. Annibali +12 more
openalex +1 more source
Understanding how and when galaxies formed stars over the history of the Universe is fundamental to the study of galaxy evolution. The star formation histories (SFHs) of galaxies in the local Universe can be measured with high precision using deep ...
Christopher T. Garling +5 more
doaj +1 more source
Diffuse Ionized Gas inside the Dwarf Irregular Galaxy NGC 6822 [PDF]
A. M. Hidalgo-Gámez, Antonio Peimbert
openalex +1 more source
Radial stellar population gradients within dwarf galaxies provide a promising avenue for disentangling the drivers of galaxy evolution, including environment. Within the Local Volume, radial stellar age gradient slopes correlate with interaction history,
Roger E. Cohen +19 more
doaj +1 more source
Spitzer 4.5 μm Luminosity-Metallicity and Mass-Metallicity Relations for Nearby Dwarf Irregular Galaxies [PDF]
H. Lee +13 more
openalex +1 more source
Chemical evolution of irregular galaxies
10 pages, 3 figs, uses moriond.sty. Review presented at XVIIIth Rencontre de Moriond `Dwarf Galaxies and Cosmology', eds.
openaire +2 more sources
Mock Observations: Morphological Analysis of Galaxies in TNG100 Simulations
In this study, we investigate the morphology of galaxies in the TNG100 simulation by applying mock observation techniques and compare the results with the observational data from the Sloan Digital Sky Survey (SDSS).
Jun-Yu Gong +3 more
doaj +1 more source

