We present dust yields for asymptotic giant branch (AGB) and super-asymptotic giant branch (SAGB) stars of solar metallicity. Stars with initial mass 1.5 M⊙ ≤...
-
PublicaciónAsymptotic giant branch and super-asymptotic giant branch stars: modelling dust production at solar metallicity
-
PublicaciónAsymptotic giant branch stars in the Large Magellanic Cloud: evolution of dust in circumstellar envelopes
We calculated theoretical evolutionary sequences of asymptotic giant branch (AGB) stars, including the formation and evolution of dust grains in their...
-
PublicaciónBalloon-Borne Submillimeter Polarimetry of the Vela C Molecular Cloud: Systematic Dependence of Polarization Fraction on Column Density and Local Polarization-Angle Dispersion
We present results for Vela C obtained during the 2012 flight of the Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry. We mapped polarized...
-
PublicaciónBroad-band spectral energy distribution of the X-ray transient Swift J1745-26 from outburst to quiescence
Aims: We aim to analyse our study of the X-ray transient Swift J1745-26, using observations obtained from its outburst in September 2012, up to its decay...
-
PublicaciónComparing Submillimeter Polarized Emission with Near-infrared Polarization of Background Stars for the Vela C Molecular Cloud
We present a large-scale combination of near-infrared (near-IR) interstellar polarization data from background starlight with polarized emission data at...
-
PublicaciónComparison of Magnetic Field Structures on Different Scales in and around the Filamentary Dark Cloud GF 9
New visible polarization data combined with existing IR and FIR polarization data are used to study how the magnetic field threading the filamentary molecular...
-
PublicaciónComparison of star formation rates from Hα and infrared luminosity as seen by Herschel
We empirically MD test the relation between the SFR(LIR) derived from the infrared luminosity, LIR, and the SFR(Hα) derived from the Hα emission line luminosity...
-
PublicaciónConstraints on spinning dust towards Galactic targets with the Very Small Array: a tentative detection of excess microwave emission towards 3C396
We present results from observations made at 33 GHz with the Very Small Array (VSA) telescope towards potential candidates in the Galactic plane for spinning...
-
PublicaciónConstraints on the dust extinction law of the Galaxy with Swift/UVOT, Gaia, and 2MASS
We explore variations of the dust extinction law of the Milky Way by selecting stars from the Swift/UVOT Serendipitous Source Catalogue, cross-matched with Gaia...