Search Results - "Blanc, Guillermo A."
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IZI: INFERRING THE GAS PHASE METALLICITY ( Z ) AND IONIZATION PARAMETER ( q ) OF IONIZED NEBULAE USING BAYESIAN STATISTICS
Published in The Astrophysical journal (10-01-2015)“…We present a new method for inferring the metallicity (Z) and ionization parameter (q) of H II regions and star-forming galaxies using strong nebular emission…”
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Distances to PHANGS galaxies: New tip of the red giant branch measurements and adopted distances
Published in Monthly notices of the Royal Astronomical Society (01-03-2021)“…ABSTRACT PHANGS-HST is an ultraviolet-optical imaging survey of 38 spiral galaxies within ∼20 Mpc. Combined with the PHANGS-ALMA, PHANGS-MUSE surveys and other…”
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Cloud-scale Molecular Gas Properties in 15 Nearby Galaxies
Published in The Astrophysical journal (20-06-2018)“…We measure the velocity dispersion, , and surface density, , of the molecular gas in nearby galaxies from CO spectral line cubes with spatial resolution 45-120…”
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Cloud-scale ISM Structure and Star Formation in M51
Published in The Astrophysical journal (01-09-2017)“…We compare the structure of molecular gas at 40 pc resolution to the ability of gas to form stars across the disk of the spiral galaxy M51. We break the PAWS…”
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Dynamical Equilibrium in the Molecular ISM in 28 Nearby Star-forming Galaxies
Published in The Astrophysical journal (01-04-2020)“…We compare the observed turbulent pressure in molecular gas, Pturb, to the required pressure for the interstellar gas to stay in equilibrium in the…”
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The Gas-Star Formation Cycle in Nearby Star-forming Galaxies. I. Assessment of Multi-scale Variations
Published in The Astrophysical journal (10-12-2019)“…The processes regulating star formation in galaxies are thought to act across a hierarchy of spatial scales. To connect extragalactic star formation relations…”
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On the duration of the embedded phase of star formation
Published in Monthly notices of the Royal Astronomical Society (01-06-2021)“…ABSTRACT Feedback from massive stars plays a key role in molecular cloud evolution. After the onset of star formation, the young stellar population is exposed…”
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LATIS: The Stellar Mass–Metallicity Relation of Star-forming Galaxies at z ∼ 2.5
Published in The Astrophysical journal (01-01-2024)“…Abstract We present the stellar mass–stellar metallicity relation for 3491 star-forming galaxies at 2 ≲ z ≲ 3 using rest-frame far-ultraviolet spectra from the…”
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Millimeter-wave Line Ratios and Sub-beam Volume Density Distributions
Published in The Astrophysical journal (01-02-2017)“…We explore the use of mm-wave emission line ratios to trace molecular gas density when observations integrate over a wide range of volume densities within a…”
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The VIRUS-P Exploration of Nearby Galaxies (VENGA): spatially resolved gas-phase metallicity distributions in barred and unbarred spirals
Published in Monthly notices of the Royal Astronomical Society (21-10-2016)“…We present a study of the excitation conditions and metallicity of ionized gas (Z gas) in eight nearby barred and unbarred spiral galaxies from the VIRUS-P…”
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LATIS: Constraints on the Galaxy–Halo Connection at z ∼ 2.5 from Galaxy–Galaxy and Galaxy–Lyα Clustering
Published in The Astrophysical journal (01-01-2024)“…Abstract The connection between galaxies and dark matter halos is often quantified using the stellar mass–halo mass (SMHM) relation. Optical and near-infrared…”
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PHANGS–JWST First Results: Destruction of the PAH Molecules in H ii Regions Probed by JWST and MUSE
Published in Astrophysical journal. Letters (01-02-2023)“…Abstract Polycyclic aromatic hydrocarbons (PAHs) play a critical role in the reprocessing of stellar radiation and balancing the heating and cooling processes…”
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A population of ultraviolet-dim protoclusters detected in absorption
Published in Nature (London) (16-06-2022)“…Galaxy protoclusters, which will eventually grow into the massive clusters we see in the local Universe, are usually traced by locating overdensities of…”
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PHANGS–JWST First Results: Duration of the Early Phase of Massive Star Formation in NGC 628
Published in Astrophysical journal. Letters (01-02-2023)“…Abstract The earliest stages of star formation, when young stars are still deeply embedded in their natal clouds, represent a critical phase in the matter…”
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Calibrating Star Formation Rate Prescriptions at Different Scales (10 pc-1 kpc) in M31
Published in The Astrophysical journal (01-03-2019)“…We calibrate commonly used star formation rate (SFR) prescriptions using observations in five kiloparsec-sized fields in the nearby galaxy Andromeda (M31) at…”
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PHANGS–JWST First Results: A Combined HST and JWST Analysis of the Nuclear Star Cluster in NGC 628
Published in Astrophysical journal. Letters (01-02-2023)“…Abstract We combine archival Hubble Space Telescope and new James Webb Space Telescope imaging data covering the ultraviolet to mid-infrared regime to…”
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Investigating the Drivers of Electron Temperature Variations in H ii Regions with Keck-KCWI and VLT-MUSE
Published in The Astrophysical journal (01-05-2024)“…Abstract H ii region electron temperatures are a critical ingredient in metallicity determinations, and recent observations have revealed systematic variations…”
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Comparing the Locations of Supernovae to CO (2–1) Emission in Their Host Galaxies
Published in The Astrophysical journal (01-02-2023)“…Abstract We measure the molecular gas environment near recent (<100 yr old) supernovae (SNe) using ∼1″ or ≤150 pc resolution CO (2–1) maps from the…”
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PHANGS-ML: Dissecting Multiphase Gas and Dust in Nearby Galaxies Using Machine Learning
Published in The Astrophysical journal (01-06-2024)“…Abstract The PHANGS survey uses Atacama Large Millimeter/submillimeter Array, Hubble Space Telescope, Very Large Telescope, and JWST to obtain an unprecedented…”
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PHANGS–JWST First Results: Interstellar Medium Structure on the Turbulent Jeans Scale in Four Disk Galaxies Observed by JWST and the Atacama Large Millimeter/submillimeter Array
Published in Astrophysical journal. Letters (01-02-2023)“…Abstract JWST/Mid-Infrared Instrument imaging of the nearby galaxies IC 5332, NGC 628, NGC 1365, and NGC 7496 from PHANGS reveals a richness of gas structures…”
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