Astrophysical: Clouds

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    Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds
    Within ten nearby (d 450 pc) Gould belt molecular clouds we evaluate statistically the relative orientation between the magnetic field projected on the plane...
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    Planetary Size Comparisons: a Photographic Study
    Not Available
  • Publication
    Planetary Size Comparisons: a Photographic Study
    Not Available
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    Polarimetry toward the IRAS Vela Shell. I. The Catalog
    We have obtained linear polarization measurements of stars along the western side of the IRAS Vela Shell toward HD 62542. From 16 CCD fields distributed along...
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    Polarimetry toward the IRAS Vela Shell. II. Extinction and Magnetic Fields
    We explore correlations between visual extinction and polarization along the western side of the Infrared Astronomical Satellite (IRAS) Vela Shell using a...
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    Polarimetry toward the Musca Dark Cloud. I. The Catalog
    We have used CCD imaging polarimetry to obtain linear polarization measurements of background stars toward the filamentary Musca dark cloud. We present a...
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    Propagation of ionizing radiation in H II regions: The effects of optically thick density fluctuations
    The accepted explanation of the observed dichotomy of two orders of magnitude between in situ measurements of electron density in H II regions, derived from...
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    Prospects for future studies using deep imaging: analysis of individual Galactic cirrus filaments
    The presence of Galactic cirrus is an obstacle for studying both faint objects in our Galaxy and low surface brightness extragalactic structures. With the aim...
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    QUIJOTE scientific results - VII. Galactic AME sources in the QUIJOTE-MFI northern hemisphere wide survey
    The QUIJOTE-MFI Northern Hemisphere Wide Survey has provided maps of the sky above declinations -30° at 11, 13, 17, and 19 GHz. These data are combined with...