Publicación
Backscattering and Line Broadening in Orion
Examination of emission lines in high-velocity-resolution optical spectra of the Orion Nebula confirms that the velocity component on the red wing of the main...
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PublicaciónBalloon 090100001: A bright, high amplitude sdB pulsatorWe report the discovery of pulsations in the light curve of Balloon 090100001, a bright sdB star (B=11.8) from the balloon-borne survey of Bixler et al. (1991)...
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PublicaciónBalloon 090100001: A short and long period pulsating sdB starWe report the discovery of long period oscillations in the light curve of the bright sdB pulsator Balloon 090100001. We find at least three peaks in the low...
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PublicaciónBalloon-Borne Submillimeter Polarimetry of the Vela C Molecular Cloud: Systematic Dependence of Polarization Fraction on Column Density and Local Polarization-Angle DispersionWe present results for Vela C obtained during the 2012 flight of the Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry. We mapped polarized...
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PublicaciónBalmer Filaments in Tycho’s Supernova Remnant: An Interplay between Cosmic-ray and Broad-neutral PrecursorsWe present Hα spectroscopic observations and detailed modeling of the Balmer filaments in the supernova remnant (SNR) Tycho (SN 1572). We used GH α FaS (Galaxy...
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PublicaciónBalmer lines emission region in NGC 3516: Kinematical and physical propertiesWe have studied the Balmer line shapes of NGC 3516 in order to find the structure of central Emission Line Region (ELR) and the physical parameters of the...
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PublicaciónBAM: bias assignment method to generate mock cataloguesWe present BAM: a novel Bias Assignment Method envisaged to generate mock catalogues. Combining the statistics of dark matter tracers from a high-resolution...
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PublicaciónBar ages derived for the first time in nearby galaxies: Insights into secular evolution from the TIMER sampleOnce galaxies settle their discs and become self-gravitating, stellar bars can form, driving the subsequent evolution of their host galaxy. Determining the ages...
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PublicaciónBar Evolution over the Last 8 Billion Years: A Constant Fraction of Strong Bars in the GEMS SurveyOne-third of present-day spirals host optically visible strong bars that drive their dynamical evolution. However, the fundamental question of how bars evolve...