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Published in 2019 at "Nature Astronomy"
DOI: 10.1038/s41550-019-0929-2
Abstract: The solar wind blows outwards from the Sun and forms a bubble of solar material in the interstellar medium. The heliopause (HP) is the boundary that divides the hot tenuous solar wind plasma in the…
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Keywords:
medium;
voyager plasma;
interstellar medium;
vlism ... See more keywords
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Published in 2020 at "Nature Astronomy"
DOI: 10.1038/s41550-020-1126-z
Abstract: The density structure of the interstellar medium determines where stars form and release energy, momentum and heavy elements, driving galaxy evolution 1 – 4 . Density variations are seeded and amplified by gas motion, but…
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Keywords:
velocity fluctuations;
interstellar medium;
gas;
structure ... See more keywords
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Published in 2021 at "Nature Astronomy"
DOI: 10.1038/s41550-021-01515-9
Abstract: Centre for Astrophysics Research, School of Physics, Engineering and Computer Science, University of Hertfordshire, College Lane, Hatfield AL10 9AB, UK Department of Physics and Atmospheric Science, Dalhousie University, Halifax, NS B3H 4R2, Canada National Research…
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Keywords:
interstellar medium;
astronomy;
ramp interstellar;
astrophysics ... See more keywords
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Published in 2018 at "Nature"
DOI: 10.1038/s41586-018-0329-2
Abstract: The chemical compositions of stars encode those of the gas from which they formed, providing important clues regarding the formation histories of galaxies. A powerful diagnostic is the abundance of α elements (O, Mg, Si,…
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Keywords:
interstellar medium;
type supernovae;
gas;
formation ... See more keywords
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Published in 2021 at "Nature"
DOI: 10.1038/s41586-021-03780-0
Abstract: The interstellar medium (ISM) comprises gases at different temperatures and densities, including ionized, atomic and molecular species, and dust particles1. The neutral ISM is dominated by neutral hydrogen2 and has ionization fractions of up to…
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Keywords:
interstellar medium;
ism;
solar metallicity;
chemical ... See more keywords
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Published in 2022 at "RSC Advances"
DOI: 10.1039/d2ra04351c
Abstract: The literature is still poor in theoretical and experimental, including both spectroscopic and thermodynamic data for protonated furan and protonated 2-cyanofuran and 3-cyanofuran (FH+, 2CFH+ and 3CFH+). These data are, however, crucial for astrophysicists and…
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Keywords:
cyanofurans protonated;
2cfh 3cfh;
formation cyanofurans;
protonated forms ... See more keywords
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Published in 2017 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/201526383
Abstract: Context. Molecular hydrogen (H 2) is the most abundant molecule of the interstellar medium (ISM) in gas phase and it has been assumed to exist in solid state or as coating on grains. Aims. Our…
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Keywords:
interstellar medium;
radical hydrogenation;
hydrogenation solid;
hydrogenation ... See more keywords
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Published in 2020 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/202039008
Abstract: Context. Spatially resolved observations of the ionized and molecular gas are critical for understanding the physical processes that govern the interstellar medium (ISM) in galaxies. Aims. To study the morpho-kinematic properties of the ionized and…
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Keywords:
interstellar medium;
molecular gas;
ism;
gas ... See more keywords
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Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa1554
Abstract: We use Milky Way-like chemodynamical simulations with a new treatment for dust destruction and growth to investigate how these two processes affect the properties of the interstellar medium in galaxies. We focus on the role…
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Keywords:
dust destruction;
interstellar medium;
gas;
dust ... See more keywords
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Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa879
Abstract: We present a sub-kpc resolved study of the interstellar medium properties in SDP.81, a z=3.042 strongly gravitationally lensed dusty star-forming galaxy, based on high-resolution, multi-band ALMA observations of the FIR continuum, CO ladder and the…
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Keywords:
dusty star;
forming galaxy;
interstellar medium;
star forming ... See more keywords
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Published in 2021 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stab236
Abstract: Based on high-resolution 3D data cubes from a magnetohydrodynamic (MHD) turbulence simulation, we study how to reveal the direction of the magnetic field within the optically thick interstellar medium by using the velocity gradient technique…
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Keywords:
magnetic fields;
medium;
optically thick;
interstellar medium ... See more keywords