Tipo de publicación: Con árbitro

  • Publicación
    Polarized, variable radio emission from the scallop-shell binary system DG CVn
    DG CVn is an eruptive variable star and represents the closest member of the known sample of complex periodic variables, or scallop-shell stars. Over the years...
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    Polarizing properties of grazing-incidence X-ray mirrors - Comment
    We show that grazing-incidence telescopes, like those used for X-ray imaging, present negligible instrumental polarization. This property does not depend on the...
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    Pole coordinates of the asteroid 338 Budrosa: implication for the asteroidal family 124
    Not Available
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    Polycyclic Aromatic Hydrocarbon Emission in the Central Regions of Three Seyferts and the Implication for Underlying Feedback Mechanisms
    We analyze JWST Mid-Infrared Instrument/Medium Resolution Spectrograph integral field unit observations of three Seyferts from the Galactic Activity, Torus, and...
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    Polynomial Approximants for the Calculation of Polarization Profiles in the He I 10830 Å Multiplet
    The He I multiplet at 10830 Å is formed in the incomplete Paschen-Back regime for typical conditions found in solar and stellar atmospheres. The positions and...
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    Populations of High-Luminosity Density-bounded H II Regions in Spiral Galaxies: Evidence and Implications
    We present evidence that the H II regions of high luminosity in disk galaxies may be density bounded, so that a significant fraction of the ionizing photons...
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    PORTA: A three-dimensional multilevel radiative transfer code for modeling the intensity and polarization of spectral lines with massively parallel computers
    The interpretation of the intensity and polarization of the spectral line radiation produced in the atmosphere of the Sun and of other stars requires solving a...
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    Portrait of the Polana-Eulalia family complex: Surface homogeneity revealed from near-infrared spectroscopy
    The inner asteroid belt is an important source of near-Earth asteroids (NEAs). Dynamical studies of the inner asteroid belt have identified several families...
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    Position-dependent infrared spectroscopy of M82 - 100,000 Orion nebulae?
    It is reported that 8-13-micron spectra have been obtained at several positions across the extended emission region of M82. No major differences among the...