Results 71 to 80 of about 4,398 (186)
Abstract Volatile‐rich xenolithic clasts in different types of brecciated meteorites represent unique pristine solar system material. This study investigates the maturity and thermal history of organic matter using Raman spectroscopy and aqueous alteration effects using infrared spectroscopy in the matrix of 15 volatile‐rich clasts (C1 and CM‐like ...
Swarna Prava Das +7 more
wiley +1 more source
Abstract Amorphous carbon (αC) is found in various extraterrestrial particles, including those thought to originate from the outer Solar System. αC can form through two main processes involving C‐rich materials: exposure to energetic charged particles and thermal processing.
M. Germanà +10 more
wiley +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
Shocks in the Very Local Interstellar Medium. [PDF]
Mostafavi P +12 more
europepmc +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
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
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
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
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
Gas-phase formation of the resonantly stabilized 1-indenyl (C9H7•) radical in the interstellar medium. [PDF]
Yang Z +9 more
europepmc +1 more source

