Articles with "interstellar medium" as a keyword



Photo from wikipedia

Voyager 2 plasma observations of the heliopause and interstellar medium

Sign Up to like & get
recommendations!
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… read more here.

Keywords: medium; voyager plasma; interstellar medium; vlism ... See more keywords
Photo from wikipedia

Ubiquitous velocity fluctuations throughout the molecular interstellar medium

Sign Up to like & get
recommendations!
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… read more here.

Keywords: velocity fluctuations; interstellar medium; gas; structure ... See more keywords
Photo by supuloo from unsplash

The ramp-up of interstellar medium enrichment at z > 4

Sign Up to like & get
recommendations!
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… read more here.

Keywords: interstellar medium; astronomy; ramp interstellar; astrophysics ... See more keywords
Photo from wikipedia

The formation of solar-neighbourhood stars in two generations separated by 5 billion years

Sign Up to like & get
recommendations!
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,… read more here.

Keywords: interstellar medium; type supernovae; gas; formation ... See more keywords
Photo from wikipedia

Large metallicity variations in the Galactic interstellar medium.

Sign Up to like & get
recommendations!
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… read more here.

Keywords: interstellar medium; ism; solar metallicity; chemical ... See more keywords
Photo by richardrschunemann from unsplash

On the formation of 2- and 3-cyanofurans and their protonated forms in interstellar medium conditions: quantum chemical evidence

Sign Up to like & get
recommendations!
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… read more here.

Keywords: cyanofurans protonated; 2cfh 3cfh; formation cyanofurans; protonated forms ... See more keywords
Photo from wikipedia

CN radical hydrogenation from solid H2 reactions, an alternative way of HCN formation in the interstellar medium

Sign Up to like & get
recommendations!
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… read more here.

Keywords: interstellar medium; radical hydrogenation; hydrogenation solid; hydrogenation ... See more keywords
Photo from wikipedia

VALES: VII. Molecular and ionized gas properties in the pressure balanced interstellar medium of starburst galaxies at z ∼ 0.15

Sign Up to like & get
recommendations!
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… read more here.

Keywords: interstellar medium; molecular gas; ism; gas ... See more keywords
Photo from wikipedia

The role of dust destruction and dust growth in the evolution of the interstellar medium

Sign Up to like & get
recommendations!
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… read more here.

Keywords: dust destruction; interstellar medium; gas; dust ... See more keywords
Photo from wikipedia

Full of Orions: a 200-pc mapping of the interstellar medium in the redshift-3 lensed dusty star-forming galaxy SDP.81

Sign Up to like & get
recommendations!
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… read more here.

Keywords: dusty star; forming galaxy; interstellar medium; star forming ... See more keywords
Photo from wikipedia

Statistical tracing of turbulent magnetic fields in the optically thick interstellar medium

Sign Up to like & get
recommendations!
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… read more here.

Keywords: magnetic fields; medium; optically thick; interstellar medium ... See more keywords