Search Results - "WOLFIRE, Mark"
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Photodissociation and X-Ray-Dominated Regions
Published in Annual review of astronomy and astrophysics (18-08-2022)“…The radiation from stars and active galactic nuclei (AGNs) creates photodissociation regions (PDRs) and X-ray-dominated regions (XDRs), where the chemistry or…”
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The Cosmic-Ray Ionization Rate in the Galactic Disk, as Determined from Observations of Molecular Ions
Published in The Astrophysical journal (20-08-2017)“…We have obtained estimates for the cosmic-ray ionization rate (CRIR) in the Galactic disk, using a detailed model for the physics and chemistry of diffuse…”
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3
The PhotoDissociation Region Toolbox: Software and Models for Astrophysical Analysis
Published in The Astronomical journal (01-01-2023)“…The PhotoDissociation Region Toolbox provides comprehensive, easy-to-use, public software tools and models that enable an understanding of the interaction of…”
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A Simple and Accurate Network for Hydrogen and Carbon Chemistry in the Interstellar Medium
Published in The Astrophysical journal (01-07-2017)“…Chemistry plays an important role in the interstellar medium (ISM), regulating the heating and cooling of the gas and determining abundances of molecular…”
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5
The Dark Molecular Gas
Published in The Astrophysical journal (20-06-2010)“…The mass of molecular gas in an interstellar cloud is often measured using line emission from low rotational levels of CO, which are sensitive to the CO mass,…”
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The CO-to-H2 Conversion Factor
Published in Annual review of astronomy and astrophysics (18-08-2013)“…CO line emission represents the most accessible and widely used tracer of the molecular ISM. This renders the translation of observed CO intensity into total H…”
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THE CHEMISTRY OF INTERSTELLAR ARGONIUM AND OTHER PROBES OF THE MOLECULAR FRACTION IN DIFFUSE CLOUDS
Published in The Astrophysical journal (01-08-2016)“…ABSTRACT We present a general parameter study in which the abundance of interstellar argonium (ArH+) is predicted using a model for the physics and chemistry…”
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The PAH Emission Characteristics of the Reflection Nebula NGC 2023
Published in The Astrophysical journal (20-02-2017)“…We present 5-20 m spectral maps of the reflection nebula NGC 2023 obtained with the Infrared Spectrograph SL and SH modes on board the Spitzer Space Telescope,…”
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The Chemistry of Interstellar Molecules Containing the Halogen Elements
Published in The Astrophysical journal (01-12-2009)“…Although they are only minor constituents of the interstellar medium, halogen-containing molecules are of special interest because of their unique…”
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[Si II], [Fe II], [C II], and H2 Emission from Massive Star-forming Regions
Published in The Astrophysical journal (10-06-2006)Get full text
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The Chemistry of Chlorine-bearing Species in the Diffuse Interstellar Medium, and New SOFIA/GREAT Observations of HCl
Published in The Astrophysical journal (01-08-2021)“…We have revisited the chemistry of chlorine-bearing species in the diffuse interstellar medium with new observations of the HCl + molecular ion and new…”
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The Densities in Diffuse and Translucent Molecular Clouds: Estimates from Observations of C2 and from Three-dimensional Extinction Maps
Published in The Astrophysical journal (01-10-2024)“…Newly computed collisional rate coefficients for the excitation of C2 in collisions with H2, presented recently by Najar & Kalugina, are significantly larger…”
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Formation of the methyl cation by photochemistry in a protoplanetary disk
Published in Nature (London) (07-09-2023)“…Forty years ago, it was proposed that gas-phase organic chemistry in the interstellar medium can be initiated by the methyl cation CH 3 + (refs. 1 – 3 ), but…”
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The Structure of Dark Molecular Gas in the Galaxy. II. Physical State of "CO-dark" Gas in the Perseus Arm
Published in The Astrophysical journal (01-10-2019)“…We report the results from a new, highly sensitive (ΔTmb ∼ 3 mK) survey for thermal OH emission at 1665 and 1667 MHz over a dense, 9 × 9 pixel grid covering a…”
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SOFIA FEEDBACK Survey: The Pillars of Creation in [C ii] and Molecular Lines
Published in The Astronomical journal (01-12-2023)“…We investigate the physical structure and conditions of photodissociation regions (PDRs) and molecular gas within the Pillars of Creation in the Eagle Nebula…”
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Velocity-resolved [ ] Emission from Cold Diffuse Clouds in the Interstellar Medium
Published in The Astrophysical journal (01-04-2018)“…We have combined emission from the 158 m fine structure transition of C+ observed with the GREAT and upGREAT instruments on SOFIA with 21 cm absorption spectra…”
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Neutral Atomic Phases of the Interstellar Medium in the Galaxy
Published in The Astrophysical journal (10-04-2003)Get full text
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Experimental Determination of the Dissociative Recombination Rate Coefficient for Rotationally Cold CH+ and Its Implications for Diffuse Cloud Chemistry
Published in The Astrophysical journal (01-11-2022)“…Observations of CH + are used to trace the physical properties of diffuse clouds, but this requires an accurate understanding of the underlying CH + chemistry…”
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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)“…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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Modeling Ionized Gas in the Small Magellanic Cloud: The Wolf–Rayet Nebula N76
Published in The Astrophysical journal (01-07-2024)“…We present Cloudy modeling of infrared emission lines in the Wolf–Rayet (WR) nebula N76 caused by one of the most luminous and hottest WR stars in the low…”
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