Results 21 to 30 of about 13,165 (147)

Dust destruction at high galactic altitude [PDF]

open access: yesАстрономия и исследование космического пространства: Всероссийская с международным участием научная конференция студентов и молодых ученых, посвященная памяти Полины Евгеньевны Захаровой, 2021
The possibility of destruction carbonaceous dust particles swept out by the radiation pressure into near-galactic space due to the relative motion of dust particles of various sizes is considered. The earlier model of the motion of dust in the Galaxy under the action of radiation pressure, gravity, and gas resistance is expanded taking into account the
E. E. Sivkova, D. Z. Wiebe
openaire   +1 more source

Effects of Barnett Magnetic Dipole–Dipole Interaction on Grain Growth and Destruction

open access: yesThe Astrophysical Journal, 2023
Rapidly spinning magnetic grains can acquire large magnetic dipole moments due to the Barnett effect. Here we study the new effect of Barnett magnetic dipole–dipole interaction on grain–grain collisions and grain growth, assuming that grains are spun up ...
Thiem Hoang, Bao Truong
doaj   +1 more source

The Dynamics, Destruction, and Survival of Supernova-formed Dust Grains [PDF]

open access: yesThe Astrophysical Journal, 2020
Abstract Observations have demonstrated that supernovae efficiently produce dust. This is consistent with the hypothesis that supernovae and asymptotic giant branch stars are the primary producers of dust in the universe. However, there has been a longstanding question of how much of the dust detected in the interiors of young supernova ...
Slavin, Jonathan D.   +3 more
openaire   +2 more sources

Modeling Dust Production, Growth, and Destruction in Reionization-era Galaxies with the CROC Simulations: Methods and Parameter Exploration

open access: yesThe Astrophysical Journal, 2022
We introduce a model for the explicit evolution of interstellar dust in a cosmological galaxy formation simulation. We post-process a simulation from the Cosmic Reionization on Computers project, integrating an ordinary differential equation for the ...
Clarke J. Esmerian, Nickolay Y. Gnedin
doaj   +1 more source

Dust sputtering within the inner heliosphere: a modelling study [PDF]

open access: yesAnnales Geophysicae, 2020
The aim of this study is to investigate through modelling how sputtering by impacting solar wind ions influences the lifetime of dust particles in the inner heliosphere near the Sun.
C. Baumann   +3 more
doaj   +1 more source

Infrared emission and the destruction of dust in HII regions [PDF]

open access: yesAstronomy Reports, 2013
accepted for publication in Astronomy Reports (2013)
Pavlyuchenkov, Yaroslav   +2 more
openaire   +2 more sources

Dust destruction at high Galactic altitude

open access: yesASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES. Proceedings of the VAK-2021 conference, Aug 23–28, 2021, 2022
We consider the destruction of dust at high galactic altitudes based on an earlier developed model of the movement of dustin the Galaxy, due to the stellar radiation pressure, gravity and gas drag. The possibility of dust sweeping is consideredtaking into account its collisions with the Galactic gas and between dust particles.
M. Murga, D. Wiebe, E. Sivkova
openaire   +1 more source

Rotational Disruption of Astrophysical Dust and Ice—Theory and Applications

open access: yesGalaxies, 2020
Dust is an essential component of the interstellar medium (ISM) and plays an important role in many different astrophysical processes and phenomena.
Thiem Hoang
doaj   +1 more source

MACROSCOPIC DUST IN PROTOPLANETARY DISKS—FROM GROWTH TO DESTRUCTION [PDF]

open access: yesThe Astrophysical Journal, 2014
11 pages, 14 ...
Deckers, Johannes, Teiser, Jens
openaire   +2 more sources

Dust Destruction in the Interstellar Medium [PDF]

open access: yesSymposium - International Astronomical Union, 1989
Grains are injected into the interstellar medium (ISM) from evolved stars and supernovae; in addition, supernova ejecta may condense onto pre-existing grains before becoming well-mixed with the interstellar gas. Once in the ISM, grains can grow by accretion, but are also subject to destruction by interstellar shocks. The current status of the theory of
openaire   +1 more source

Home - About - Disclaimer - Privacy