Search Results - "Dalcanton, Julianne"
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Nebular Continuum and Line Emission in Stellar Population Synthesis Models
Published in The Astrophysical journal (01-05-2017)“…Accounting for nebular emission when modeling galaxy spectral energy distributions (SEDs) is important, as both line and continuum emissions can contribute…”
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Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback
Published in Nature (London) (01-05-2019)“…The physics of star formation and the deposition of mass, momentum and energy into the interstellar medium by massive stars (‘feedback’) are the main…”
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3
THE STAR FORMATION HISTORIES OF LOCAL GROUP DWARF GALAXIES. I. HUBBLE SPACE TELESCOPE/WIDE FIELD PLANETARY CAMERA 2 OBSERVATIONS
Published in The Astrophysical journal (10-07-2014)“…We present uniformly measured star formation histories (SFHs) of 40 Local Group (LG) dwarf galaxies based on color-magnitude diagram (CMD) analysis from…”
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The Metallicity of Galaxy Disks: Infall versus Outflow
Published in The Astrophysical journal (01-04-2007)“…Both gas accretion (infall) and winds (outflow) change a galaxy's metallicity and gas fraction, lowering the effective yield. Low effective yields in galaxies…”
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EVOLUTION OF THERMALLY PULSING ASYMPTOTIC GIANT BRANCH STARS. V. CONSTRAINING THE MASS LOSS AND LIFETIMES OF INTERMEDIATE-MASS, LOW-METALLICITY AGB STARS
Published in The Astrophysical journal (10-05-2016)“…ABSTRACT Thermally pulsing asymptotic giant branch (TP-AGB) stars are relatively short lived (less than a few Myr), yet their cool effective temperatures, high…”
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THE STAR FORMATION HISTORIES OF LOCAL GROUP DWARF GALAXIES. II. SEARCHING FOR SIGNATURES OF REIONIZATION
Published in The Astrophysical journal (10-07-2014)“…We search for signatures of reionization in the star formation histories (SFHs) of 38 Local Group dwarf galaxies (10 super(4) < M sub([sstarf]) < 10 super(9) M…”
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EXPLORING SYSTEMATIC EFFECTS IN THE RELATION BETWEEN STELLAR MASS, GAS PHASE METALLICITY, AND STAR FORMATION RATE
Published in The Astrophysical journal (10-08-2016)“…ABSTRACT There is evidence that the well-established mass-metallicity relation in galaxies is correlated with a third parameter: star formation rate (SFR). The…”
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Stellar and Nebular Diagnostics in the Ultraviolet for Star-forming Galaxies
Published in The Astrophysical journal (10-08-2018)“…There is a long history of using optical emission and absorption lines to constrain the metallicity and ionization parameters of gas in galaxies. However,…”
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Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Small Magellanic Cloud
Published in Monthly notices of the Royal Astronomical Society (01-06-2019)“…Abstract The thermally pulsing asymptotic giant branch (TP-AGB) experienced by low- and intermediate-mass stars is one of the most uncertain phases of stellar…”
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Panchromatic Hubble Andromeda Treasury. XVIII. The High-mass Truncation of the Star Cluster Mass Function
Published in The Astrophysical journal (20-04-2017)“…We measure the mass function for a sample of 840 young star clusters with ages between 10 and 300 Myr observed by the Panchromatic Hubble Andromeda Treasury…”
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THE STAR FORMATION HISTORIES OF LOCAL GROUP DWARF GALAXIES. III. CHARACTERIZING QUENCHING IN LOW-MASS GALAXIES
Published in The Astrophysical journal (10-05-2015)“…We explore the quenching of low-mass galaxies (10 super(4) [<, ~] M[lowstar] [<, ~] 10 super(8) M sub([middot in circle])) as a function of lookback time using…”
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A NEW GENERATION OF PARSEC-COLIBRI STELLAR ISOCHRONES INCLUDING THE TP-AGB PHASE
Published in The Astrophysical journal (20-01-2017)“…We introduce a new generation of PARSEC-COLIBRI stellar isochrones that includes a detailed treatment of the thermally pulsing asymptotic giant branch (TP-AGB)…”
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Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Large Magellanic Cloud
Published in Monthly notices of the Royal Astronomical Society (01-11-2020)“…ABSTRACT Reliable models of the thermally pulsing asymptotic giant branch (TP-AGB) phase are of critical importance across astrophysics, including our…”
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Stellar Feedback and Resolved Stellar IFU Spectroscopy in the Nearby Spiral Galaxy NGC 300
Published in The Astrophysical journal (01-03-2020)“…We present MUSE integral field unit (IFU) observations of five individual H ii regions in two giant star-forming complexes in the low-metallicity, nearby dwarf…”
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Constraints for the Progenitor Masses of Historic Core-collapse Supernovae
Published in The Astrophysical journal (10-06-2018)“…We age-date the stellar populations associated with 12 historic nearby core-collapse supernovae (CCSNe) and two supernova impostors; from these ages, we infer…”
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PHAT. XIX. The Ancient Star Formation History of the M31 Disk
Published in The Astrophysical journal (10-09-2017)“…We map the star formation history across M31 by fitting stellar evolution models to color-magnitude diagrams of each 83″ × 83″ (0.3 × 1.4 kpc, deprojected)…”
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The Panchromatic Hubble Andromeda Treasury. XX. The Disk of M31 is Thick
Published in The Astronomical journal (01-08-2023)“…Abstract We present a new approach to measuring the thickness of a partially face-on stellar disk, using dust geometry. In a moderately-inclined disk galaxy,…”
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A Multiwavelength Classification and Study of Red Supergiant Candidates in NGC 6946
Published in The Astrophysical journal (01-03-2023)“…Abstract We have combined resolved stellar photometry from Hubble Space Telescope (HST), Spitzer, and Gaia to identify red supergiant (RSG) candidates in NGC…”
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Spatially Resolved Metal Loss from M31
Published in The Astrophysical journal (01-06-2019)“…As galaxies evolve, they must enrich and exchange gas with the surrounding medium, but the timing of these processes and how much gas is involved remain poorly…”
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KPM: A Flexible and Data-driven K-process Model for Nucleosynthesis
Published in The Astronomical journal (01-03-2024)“…Abstract The element abundance pattern found in Milky Way disk stars is close to two-dimensional, dominated by production from one prompt process and one…”
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