Search Results - "Jameson, Katherine E"
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First Results from the Herschel and ALMA Spectroscopic Surveys of the SMC: The Relationship between [C ii]-bright Gas and CO-bright Gas at Low Metallicity
Published in The Astrophysical journal (01-02-2018)“…Abstract The Small Magellanic Cloud (SMC) provides the only laboratory to study the structure of molecular gas at high resolution and low metallicity. We…”
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Journal Article -
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First extragalactic measurement of the turbulence driving parameter: ALMA observations of the star-forming region N159E in the Large Magellanic Cloud
Published in Monthly notices of the Royal Astronomical Society (21-10-2021)“…ABSTRACT Studying the driving modes of turbulence is important for characterizing the impact of turbulence in various astrophysical environments. The driving…”
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Journal Article -
3
THE RELATIONSHIP BETWEEN MOLECULAR GAS, H i, AND STAR FORMATION IN THE LOW-MASS, LOW-METALLICITY MAGELLANIC CLOUDS
Published in The Astrophysical journal (01-07-2016)“…ABSTRACT The Magellanic Clouds provide the only laboratory to study the effects of metallicity and galaxy mass on molecular gas and star formation at high ( 20…”
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Journal Article -
4
Sequential Star Formation in the Young SMC Region NGC 602: Insights from ALMA
Published in The Astrophysical journal (01-10-2022)“…Abstract NGC 602 is a young, low-metallicity star cluster in the “Wing” of the Small Magellanic Cloud. We reveal the recent evolutionary past of the cluster…”
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Journal Article -
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First Results from the Herschel and ALMA Spectroscopic Surveys of the SMC: The Relationship between [C ii]-bright Gas and CO-bright Gas at Low Metallicity ∗ Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA
Published in The Astrophysical journal (30-01-2018)“…The Small Magellanic Cloud (SMC) provides the only laboratory to study the structure of molecular gas at high resolution and low metallicity. We present…”
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Journal Article -
6
Molecular gas and star formation at low metallicity in the Magellanic Clouds
Published 01-01-2016“…The Magellanic Clouds are two interacting, gas-rich, star-forming, low-mass, nearby satellite galaxies of the Milky Way that afford a unique view of…”
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Dissertation -
7
Sequential Star Formation in the Young SMC Region NGC 602: Insights from ALMA
Published 29-08-2022“…NGC 602 is a young, low-metallicity star cluster in the "Wing" of the Small Magellanic Cloud. We reveal the recent evolutionary past of the cluster through…”
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Journal Article -
8
First extragalactic measurement of the turbulence driving parameter: ALMA observations of the star-forming region N159E in the Large Magellanic Cloud
Published 19-10-2021“…Studying the driving modes of turbulence is important for characterizing the impact of turbulence in various astrophysical environments. The driving mode of…”
Get full text
Journal Article -
9
First Results from the $Herschel$ and ALMA Spectroscopic Surveys of the SMC: The Relationship Between [CII]-bright Gas and CO-bright Gas at Low Metallicity
Published 10-01-2018“…The Small Magellanic Cloud (SMC) provides the only laboratory to study the structure of molecular gas at high resolution and low metallicity. We present…”
Get full text
Journal Article -
10
The Relationship Between Molecular Gas, HI, and Star Formation in the Low-Mass, Low-Metallicity Magellanic Clouds
Published 25-04-2016“…The Magellanic Clouds provide the only laboratory to study the effect of metallicity and galaxy mass on molecular gas and star formation at high (~20 pc)…”
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Journal Article