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The Small-scale Dynamo in a Multiphase Supernova-driven Medium
The Astrophysical Journal, 2023 Magnetic fields grow quickly, even at early cosmological times, suggesting the action of a small-scale dynamo (SSD) in the interstellar medium (ISM) of galaxies. Many studies have focused on idealized, isotropic, homogeneous, turbulent driving of the SSD.
Frederick A. Gent +3 more
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Frontiers in Astronomy and Space Sciences, 2023 The recently published Interstellar Probe (ISP) study report describes a pragmatic mission concept with a launch window that starts in 2036 and is expected to reach several hundreds of astronomical units past the heliopause within a time frame of ≥50 ...
K. Dialynas +30 more
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Multi-line Observations, Models, and Data Needed to Understand the Nature of UV-irradiated Interstellar Matter [PDF]
EPJ Web of Conferences, 2022 Far-ultraviolet photons from OB-type massive stars regulate the heating, ionization, and chemistry of much of the neutral interstellar gas in star-forming galaxies.
Goicoechea Javier R. +2 more
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Grain Dynamics in Magnetized Interstellar Gas [PDF]
The Astrophysical Journal, 2002 11 pages, 1 figure, ApJL, in ...
Lazarian, A., Yan, Huirong
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DYNAMIC SPECTRAL MAPPING OF INTERSTELLAR PLASMA LENSES [PDF]
The Astrophysical Journal, 2016 ABSTRACT Compact radio sources sometimes exhibit intervals of large, rapid changes in their flux density, due to lensing by interstellar plasma crossing the line of sight. A novel survey program has made it possible to discover these “Extreme Scattering Events” (ESEs) in real time, resulting in a high-quality dynamic spectrum of an ESE ...
Artem V. Tuntsov +7 more
openaire +3 more sources
The Influence of Outflow Feedback in Clumps
The Astrophysical Journal, 2023 We analyzed the influence of outflow feedback from two perspectives: turbulent support and potential disruptive effect, of which 694 clumps and 188 have been identified as outflow candidates.
Qiang Li +5 more
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The Astrophysical Journal Supplement Series, 2023 Gas infall motions play a crucial role in high-mass star formation and are characterized by observable signatures of blueshifted asymmetric spectral line profiles (“blue profiles”).
Fengwei Xu +5 more
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Aspects of the Mass Distribution of Interstellar Dust Grains in the Solar System from In-Situ Measurements [PDF]
, 1999 The in-situ detection of interstellar dust grains in the Solar System by the dust instruments on-board the Ulysses and Galileo spacecraft as well as the recent measurements of hyperbolic radar meteors give information on the properties of the ...
Baggaley +30 more
core +2 more sources
High-mass Starless Clumps: Dynamical State and Correlation between Physical Parameters
The Astrophysical Journal, 2023 In order to study the initial conditions of massive star formation, we have previously built a sample of 463 high-mass starless clumps (HMSCs) across the inner Galactic plane covered by multiple continuum surveys.
Bo Huang +5 more
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The Astrophysical Journal, 2023 We present Stratospheric Observatory For Infrared Astronomy (SOFIA) + Atacama Large Millimeter/submillimeter Array (ALMA) continuum and spectral-line polarization data on the massive molecular cloud BYF 73, revealing important details about the magnetic ...
Peter J. Barnes +6 more
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