Astrophysical: Clouds

  • Publication
    Comparison of Prestellar Core Elongations and Large-scale Molecular Cloud Structures in the Lupus I Region
    Turbulence and magnetic fields are expected to be important for regulating molecular cloud formation and evolution. However, their effects on sub-parsec to 100...
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    Discovery of TeV γ-ray emission from the neighbourhood of the supernova remnant G24.7+0.6 by MAGIC
    SNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In the GeV regime, SNR G24.7+0.6 (3FHL J1834.1-0706e/FGES J1834.1-0706...
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    Dust and Magnetic Field in Dense Regions of the Interstellar Medium
    Not Available
  • Publication
    Earth's albedo variations 1998-2014 as measured from ground-based earthshine observations
    The Earth's albedo is a fundamental climate parameter for understanding the radiation budget of the atmosphere. It has been traditionally measured not only from...
  • Publication
    Effects of photon escape on diagnostic diagrams for H II regions
    In this article we first outline the mounting evidence that a significant fraction of the ionizing photons emitted by OB stars within H ii regions escape from...
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    Electric Dipole Emission by Fulleranes and Galactic Anomalous Microwave Emission
    We study the rotation rates and electric dipole emission of hydrogenated icosahedral fullerenes (single and multishell) in various phases of the interstellar...
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    Erratum: Small-scale clustering of nano-dust grains in supersonic turbulence
  • Publication
    Evidence for the Large-Scale Dissociation of Molecular Gas in the Inner Spiral Arms of M81
    We compare the detailed distributions of H I, H alpha , and 150 nm far-UV (FUV) continuum emission in the spiral arms of M81 at a resolution of 9" (linear...
  • Publication
    Fast-to-Alfvén Mode Conversion Mediated by the Hall Current. I. Cold Plasma Model
    The photospheric temperature minimum in the Sun and solar-like stars is very weakly ionized, with an ionization fraction f as low as 10‑4. In galactic star...