Results 121 to 130 of about 402,386 (219)
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
Discussion on Irregular Galaxies [PDF]
openaire +1 more source
The inclination of the dwarf irregular galaxy Holmberg II
We provide constraints on the inclination angle of the H\,{\sc i} disk of the dwarf irregular galaxy Holmberg II (Ho II) from stability analysis of the outer gaseous disk. We point out that a mean inclination angle of 27 degrees and thus a flat circular velocity of ~60 km/s, is required to have a level of gravitational stability similar to that found ...
F. J. Sánchez-Salcedo +2 more
openaire +3 more sources
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
HegemanLab/galaxy-tardis: First release of Galaxy TARDIS with DEMO
First release of Galaxy TARDIS with DEMO <p>The DEMO script is not yet self-contained because it requires an external S3 server to demonstrate the backup and restore functionality - I am deferring this to the next release.</p> <p>Please
Arthur Eschenlauer
core +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
Emission Line Velocity Field Of The Magellanic Irregular Galaxy Ngc 4449
The imaging spectroscopic observations of the Magellanic irregular galaxy NGC 4449 were made to show the detailed kinematic structure of the galaxy. Many filamentary structures and Several bubble-like structures are recognized in a 3D data cube of Hff ...
Minoru Sasaki +5 more
core
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
The Galaxy UV Legacy Project (GULP) is a Cycle 28 Treasury program with the Hubble Space Telescope designed to characterize resolved massive stars, OB associations, and young star clusters in 26 nearby star-forming galaxies. Utilizing the Advanced Camera
E. Sabbi +20 more
doaj +1 more source
Context. The impact of extremely low-density environments such as the diffuse intergalactic medium (IGM) on the neutral gas distribution of dwarf galaxies remains poorly explored observationally. Aims.
Namumba Brenda +14 more
doaj +1 more source

