Modelling ultraviolet-line diagnostics of stars, the ionized and the neutral interstellar medium in star-forming galaxies

2017/05/27 by A. Vidal-García, Alba Vidal-García, S. Charlot +4 · 1 citation
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #Galaxy #Interstellar medium #Ion #Ionization #Line (geometry) #Optics #Physics #Star (game theory) #Stars #Stellar, planetary, and galactic studies #Ultraviolet #astro-ph.GA

paper · pdf · doi:10.1093/mnras/stx1324

published as Monthly Notices of the Royal Astronomical Society, Volume 470, Issue 3, 21 September 2017, Pages 3532-3556 · 27 pages, 21 figures. Accepted for publication in MNRAS

openalex publication_date 2017/05/27 · arxiv created 2017/09/14 · arxiv updated 2017/09/15 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

International audience

Citations

• The SIMBAD astronomical database
• parsec evolutionary tracks of massive stars up to 350 M⊙at metallicities 0.0001 ≤Z≤ 0.04
• Synthetic Mid‐UV Spectroscopic Indices of Stars
• The interstellar environment of our galaxy
• THE PRESENT-DAY STAR FORMATION RATE OF THE MILKY WAY DETERMINED FROM SPITZER -DETECTED YOUNG STELLAR OBJECTS
• Spectral Modeling of Star‐forming Regions in the Ultraviolet: Stellar Metallicity Diagnostics for High‐Redshift Galaxies
• An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent
• Starburst99: Synthesis Models for Galaxies with Active Star Formation
• New Observations of the Interstellar Medium in the Lyman Break Galaxy MS 1512−cB58
• STAR FORMATION EFFICIENCIES AND LIFETIMES OF GIANT MOLECULAR CLOUDS IN THE MILKY WAY
• Surface brightness profiles and structural parameters for 53 rich stellar clusters in the Large Magellanic Cloud
• A Grid of Non‐LTE Line‐blanketed Model Atmospheres of O‐Type Stars
• parsec: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code
• A Grid of NLTE Line‐blanketed Model Atmospheres of Early B‐Type Stars
• Galactic Stellar and Substellar Initial Mass Function
• Mass-loss predictions for O and B stars as a function of metallicity
• The Galactic WN stars
• Rest‐Frame Ultraviolet Spectra of \documentclassaastex \usepackageamsbsy \usepackageamsfonts \usepackageamssymb \usepackagebm \usepackagemathrsfs \usepackagepifont \usepackagestmaryrd \usepackagetextcomp \usepackageportland,xspace \usepackageamsmath,amsxtra \usepackage[OT2,OT1]fontenc \newcommand\cyr \renewcommand\rmdefaultwncyr \renewcommand\sfdefaultwncyss \renewcommand\encodingdefaultOT2 \normalfont \selectfont \DeclareTextFontCommand\textcyr\cyr \pagestyleempty \DeclareMathSizes10976 \begindocument \landscape z∼ 3 \enddocument Lyman Break Galaxies

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• The MUSE Deep Lensed Field on the Hubble Frontier Field MACS J0416