The Dynamics of Interstellar Asteroids and Comets within the Galaxy: An Assessment of Local Candidate Source Regions for 1I/’Oumuamua and 2I/Borisov [PDF]
Tim Hallatt, Paul Wiegert
openalex +1 more source
Dust-evacuated Zones near Massive Stars: Consequences of Dust Dynamics on Star-forming Regions
Stars form within dense cores composed of both gas and dust within molecular clouds. However, despite the crucial role that dust plays in the star formation process, its dynamics is frequently overlooked, with the common assumption being a constant ...
Nadine H. Soliman +2 more
doaj +1 more source
Formation of Interstellar Complex Polycyclic Aromatic Hydrocarbons: Insights from Molecular Dynamics Simulations of Dehydrogenated Benzene [PDF]
Meriem Hanine +6 more
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The leading mechanism for the origin of the Interstellar Boundary Explorer (IBEX) “ribbon” of enhanced energetic neutral atoms (ENAs) from the outer heliosphere is the so-called secondary ENA process.
Yifan Huang +6 more
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Implications of the interstellar object 1I/'Oumuamua for planetary dynamics and planetesimal formation [PDF]
Sean N. Raymond +4 more
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Cloud–Cloud Collision and Cluster Formation in the W5-NW Complex
We present a detailed structural and gas kinematic study of the star-forming complex W5-NW. A cloud–cloud collision scenario unravels with evidence of collision-induced star and cluster formation.
Namitha Issac +7 more
doaj +1 more source
An S-shaped Filament Formed Due to Cloud–Cloud Collision in Molecular Cloud G178.28-00.61
We present compelling observational evidence supporting G178.28-00.61 as an early-stage candidate for cloud–cloud collision (CCC), with indications of the formation of an S-shaped filament, evenly separated dense cores, and young star clusters.
Tianwei Zhang +20 more
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Detection of an Explosive Outflow in G34.26+0.15
This paper reports on the detection of a likely explosive outflow in the high-mass star-forming complex G34.26+0.15, adding to the small number (six) of explosive outflows detected so far.
Namitha Issac +8 more
doaj +1 more source
Dynamical evolution and molecular abundances of interstellar clouds
Dynamical models are presented that start with interstellar gas in an initial diffuse state and consider their gravitational collapse and the formation of dense cores. Frozen-in tangled magnetic fields are included to mimic forces that might oppose gravitational contraction and whose effectiveness may increase with increasing core densities.
Sheo S. Prasad +2 more
openaire +1 more source
An Anisotropic Plasma Model of the Heliospheric Interface
We present a pioneering model of the interaction between the solar wind and the surrounding interstellar medium that includes the possibility of different pressures in directions parallel and perpendicular to the magnetic field.
Vladimir Florinski +6 more
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