Results 81 to 90 of about 1,259 (182)
The Abundance of Mg in the Interstellar Medium
An empirical determination of the f-values of the far-UV Mg II lines at 1239 A and 1240 A is reported. The strong near-UV Mg II lines at 2796 A and 2803 A are generally highly saturated along most interstellar sightlines outside the local ISM and usually yield extremely uncertain estimates of Mg II column densities in interstellar gas.
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We report an extensive rotational spectroscopic analysis of singly deuterated methyl mercaptan (CH _2 DSH) using both millimeter and far-infrared synchrotron spectra to achieve a global torsional analysis of the three lowest torsional substates ( e _0 ...
Hayley A. Bunn +10 more
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The Impact of Hydrogen Atom Tunneling on Aromatic Chemistry in TMC-1
Hydrogen atom tunneling likely plays a substantial role in the gas-phase chemistry of astrochemical environments. To determine the potential effect that it has on the chemical modeling of aromatic molecules, we screened both the kida.uva.2024 network and
Reace H. J. Willis +4 more
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Water and methanol are key components of interstellar ices and gas in star- and planet-forming regions, but direct observations of water in low-mass protostars are challenging due to atmospheric absorption.
Curtis DeWitt +10 more
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Interstellar Abundance of the Hydrogen Molecule.
Abstract : Contents: Mechanisms for the formulation of molecular hydrogen Dissociative processes for a static interstellar medium Dissociative effects of clouds motions Summary Appendix A: Photodissociation and photoionization Appendix B: Velocity distribution of H I clouds Appendix C: Stromgren spheres Appendix D: Problem in Brownian ...
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Element Nucleosynthetic Origins from Abundance Spatial Distributions beyond the Milky Way
An element’s astrophysical origin should be reflected in the spatial distribution of its abundance, yielding measurably different spatial distributions for elements with different nucleosynthetic sites.
Zefeng Li +9 more
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Potential Nitrogen Enrichment via Direct-collapse Wolf–Rayet Stars in a z = 4.7 Star-forming Galaxy
We present analyses of a nitrogen-enriched star-forming galaxy, ID60001, at z = 4.6928 based on James Webb Space Telescope/NIRSpec Multi-Object Spectroscopy and NIRCam photometry. From rest-frame optical emission lines we derive the nitrogen-to-oxygen (N/
Yechi Zhang +2 more
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Empirically measuring the primordial He mass fraction, Y _p , requires a significant number of low-metallicity nebulae with direct constraints on He/H and O/H abundances.
Noah S. J. Rogers +9 more
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Enols represent highly reactive intermediates toward the synthesis of complex organic molecules in the interstellar medium (ISM) and serve as key tracers of nonequilibrium chemistry driven by Galactic cosmic rays.
Michela Nonne +10 more
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On the Abundance of Interstellar Beryllium.
Lyman, Jr. Spitzer, George B. Field
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