Results 61 to 70 of about 4,557 (177)
Characteristics Of The Diffuse Interstellar Medium [PDF]
There have been several recent changes in perspective on the diffuse interstellar environment, including recognition of a thick disk of warm gas, cosmic rays, and magnetic field. In addition, evidence for a pervasive hot phase driven by supernova disruption has weakened to the point that a quasihomogeneous warm intercloud gas may occupy most of the ...
openaire +1 more source
Advancing our understanding of astrophysical turbulence is bottlenecked by the limited resolution of numerical simulations that may not fully sample scales in the inertial range.
Diane M. Salim +2 more
doaj +1 more source
The Solar Magnetic Hump, Heliopause, and the Very Local Interstellar Medium
The magnetic hump was observed from 2020.4 to ∼2022 by Burlaga et al. who offered the hypothesis that it originated at the Sun during the declining phase of the solar cycle.
L. F. Burlaga +4 more
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Peptide Bonds in the Interstellar Medium: Facile Catalytic Formation from Nitriles on Water-Ice Grains. [PDF]
Kerkeni B, Simmie JM.
europepmc +1 more source
Energy Balance in the Interstellar Medium [PDF]
A large number (approximately 7) of different components or phases are needed to describe the interstellar medium. The neutral intercloud medium is probably a composite of (a) “lukewarm, substandard” clouds (heated by grain photoeffect and shockwaves), (b) the interfaces between clouds and coronal gas and (c) some “phase 2” gas heated by soft X-rays ...
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Evidence for Core–Core Collision in Barnard 68
The prestellar core Barnard 68 (B68) is a prototypical source to study the initial conditions and chemical processes of star formation. A previous numerical simulation suggested the southeastern bullet is impacting on the main body of B68.
Dalei Li +12 more
doaj +1 more source
Shocks in the Very Local Interstellar Medium. [PDF]
Mostafavi P +12 more
europepmc +1 more source
Intermittency in the Magnetic Hump in the VLISM
Voyager 1 has been moving through the very local interstellar medium (VLISM) for ∼1 solar cycle, from 122.58 au on 2012/DOY 238 (August 25) to 158.5 au on 2023.0.
L. F. Burlaga +5 more
doaj +1 more source
Future Exploration of the Outer Heliosphere and Very Local Interstellar Medium by Interstellar Probe. [PDF]
Brandt PC +42 more
europepmc +1 more source
Hunting for Complex Organic Molecules in the Interstellar Medium: The Role of Accurate Low-Cost Theoretical Geometries and Rotational Constants. [PDF]
Barone V, Lazzari F.
europepmc +1 more source

