Results 111 to 120 of about 37,732 (195)

Dust Processing in the Interstellar Medium [PDF]

open access: yesProceedings of The Life Cycle of Dust in the Universe: Observations, Theory, and Laboratory Experiments — PoS(LCDU2013), 2014
openaire   +1 more source

Plasma generation and high energy electron processing of interstellar carbonaceous dust analogs

open access: yes, 2017
Santiago de Compostela, Facultade de Química,17-21 julio 2017. -- http://www.bienalrsef2017.com/bienalrsef17/ Carbonaceous compounds are found in very diverse astronomical media [1], a significant amount consisting in small dust grains. This dust originates characteristic IR absorption bands revealing the presence of aliphatic and aromatic ...
Tanarro, Isabel   +7 more
openaire   +1 more source

Photocleavage of Aliphatic C–C Bonds in the Interstellar Medium

open access: yesThe Astrophysical Journal
Ultraviolet (UV) processing in the interstellar medium (ISM) induces the dehydrogenation of hydrocarbons. Aliphatics, including alkanes, are present in different interstellar environments, being prevalently formed in evolved stars; thus, the ...
Guillermo Tajuelo-Castilla   +8 more
doaj   +1 more source

Analogs of interstellar carbonaceous dust: processing by electron bombardment and theoretical modeling

open access: yes, 2016
Workshop on interstellar matter (ILTS Symposium); Institute of Low Temperature Science, University Sapporo, Hokkaido (Japan); 19-21 October, 2016 Observational evidence, based on IR absorption spectra, indicates that interstellar (IS) carbonaceous dust in the diffuse interstellar medium is largely made of some sort of hydrogenated amorphous
Herrero, Víctor J.   +5 more
openaire   +1 more source

Proposed Importance of HOCO Chemistry: Inefficient Formation of CO2 from CO and OH Reactions on Ice Dust

open access: yesThe Astrophysical Journal
With the advent of JWST ice observations, dedicated studies on the formation reactions of detected molecules are becoming increasingly important. One of the most interesting molecules in interstellar ice is CO _2 .
Atsuki Ishibashi   +5 more
doaj   +1 more source

Sensitivity of Polarization to Grain Shape. II. Aggregates

open access: yesThe Astrophysical Journal
A previous study (Paper I) investigated the polarization properties of a variety of simple convex grain shapes, some of which were found to be consistent with the observed polarization properties of interstellar dust from far-ultraviolet to far-infrared.
B. T. Draine
doaj   +1 more source

Probing 3D Magnetic Fields Using Thermal Dust Polarization and Grain Alignment Theory

open access: yesThe Astrophysical Journal
Magnetic fields are ubiquitous in the Universe and are thought to play an important role in various astrophysical processes. Polarization of thermal emission from dust grains aligned with the magnetic field is widely used to measure the 2D magnetic field
Thiem Hoang, Bao Truong
doaj   +1 more source

Polycyclic Aromatic Hydrocarbon Emission in the Central Regions of Three Seyferts and the Implication for Underlying Feedback Mechanisms

open access: yesThe Astrophysical Journal Letters
We analyze JWST Mid-Infrared Instrument/Medium Resolution Spectrograph integral field unit observations of three Seyferts from the Galactic Activity, Torus, and Outflow Survey (GATOS) and showcase the intriguing polycyclic aromatic hydrocarbon (PAH) and ...
Lulu Zhang   +31 more
doaj   +1 more source

The Ultraviolet Slopes of Early Universe Galaxies: The Impact of Bursty Star Formation, Dust, and Nebular Continuum Emission

open access: yesThe Astrophysical Journal
JWST has enabled the detection of the ultraviolet (UV) continuum of galaxies at z > 10, revealing extremely blue, potentially dust-free galaxies. However, interpreting UV spectra is complicated by the well-known degeneracy between stellar ages, dust ...
Desika Narayanan   +10 more
doaj   +1 more source

Binding Energies of Interstellar Complex Organic Molecules on Water Ice Surfaces: A Quantum Chemical Investigation

open access: yesThe Astrophysical Journal
Interstellar dust grains are enveloped by ices of frozen molecules in cold, dense regions of the interstellar medium (ISM), which are also observed in the gas phase. Whether a species is in the solid or gaseous state is governed by its binding energy (BE)
Harjasnoor Kakkar   +4 more
doaj   +1 more source

Home - About - Disclaimer - Privacy