Hydrocarbon analogs of cosmic dust to trace the solid carbon abundance in the interstellar medium
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics
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4. THE STRUCTURE, ORIGIN, AND EVOLUTION OF INTERSTELLAR HYDROCARBON GRAINS
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1. Redshift–luminosity characterization of active galactic nucleus galaxies having obscuring dusty material using the spectral energy distribution from the X-ray to far-infrared;Monthly Notices of the Royal Astronomical Society;2022-12-22
2. Structure and evolution of interstellar carbonaceous dust. Insights from the laboratory;Frontiers in Astronomy and Space Sciences;2022-12-08
3. Impacts of the PAH size and the radiation intensity on the IR features of illuminated dust within the reflection nebulae;Advances in Space Research;2021-06
4. OUP accepted manuscript;Monthly Notices of the Royal Astronomical Society;2021
5. Aliphatic hydrocarbon content of interstellar dust;Proceedings of the International Astronomical Union;2019-04
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