output
19922026
Showing 2010 · astro-ph.GAShow all

25 papers · 2 filters

astro-ph.GA2010★ 194 cited

Multi-Element Abundance Measurements from Medium-Resolution Spectra. II. Catalog of Stars in Milky Way Dwarf Satellite Galaxies

Evan N. Kirby, Puragra Guhathakurta, Joshua D. Simon +7

We present a catalog of Fe, Mg, Si, Ca, and Ti abundances for 2961 red giant stars that are likely members of eight dwarf satellite galaxies of the Milky Way (MW): Sculptor, Fornax…

astro-ph.GA2010★ 179 cited

Mid-Infrared Spectral Diagnostics of Luminous Infrared Galaxies

A. O. Petric, L. Armus, J. Howell +22

We present a statistical analysis of the mid-infrared (MIR) spectra of 248 luminous infrared (IR) galaxies (LIRGs) which comprise the Great Observatories All-sky LIRG Survey (GOALS…

astro-ph.GA2010★ 133 cited

Accurate dynamical mass determination of a classical Cepheid in an eclipsing binary system

G. Pietrzynski, I. B. Thompson, W. Gieren +5

Stellar pulsation theory provides a means of determining the masses of pulsating classical Cepheid supergiant - it is the pulsation that causes their luminosity to vary. Such pulsa…

astro-ph.GA2010★ 1 cited

Galactic chemical evolution: the observational side

Andrew McWilliam

In this review I outline some ideas in chemical evolution, necessary for understanding the evolution of galaxies from measured elemental abundance ratios. I then discuss abundance…

astro-ph.GA2010★ 336 cited

Multi-Element Abundance Measurements from Medium-Resolution Spectra. III. Metallicity Distributions of Milky Way Dwarf Satellite Galaxies

Evan N. Kirby, Gustavo A. Lanfranchi, Joshua D. Simon +2

We present metallicity distribution functions (MDFs) for the central regions of eight dwarf satellite galaxies of the Milky Way: Fornax, Leo I and II, Sculptor, Sextans, Draco, Can…

astro-ph.GA2010★ 132 cited

High star formation rates as the origin of turbulence in early and modern disk galaxies

Andrew W. Green, Karl Glazebrook, Peter J. McGregor +6

High spatial and spectral resolution observations of star formation and kinematics in early galaxies have shown that two-thirds are massive rotating disk galaxies with the remainde…