The Inner Abundance Gradient of M33 from Bright Planetary Nebulae
Not Available
Stasińska, Grażyna et al.
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2006
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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The hidden life of massive starsA considerable fraction of the massive stars of our galaxy is obscured by dust. Dust extinction is preventing us from using powerful criteria, developed at UV and optical wavelength ranges, to infer physical properties of hot stars. At wavelengths longwards of about 5 microns, emission from warm dust is typically dominating the spectra. It isLenorzer, A. et al.
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The Extended-UCM Survey: an Hα Approach to the Universe at different redshiftsNot AvailableGallego, J.
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The Epeakrest E correlation in GRBs in the BATSE catalogThe energy emission involved in a Gamma-Ray Burst evidently can be estimated only provided that we know the distance to the source. The same is true for the peak energy of the event in the source rest frame. Redshifts have been actually measured only for about 40 events. In order to check if it is possible to extend the Epeakrest E relationPizzichini, G. et al.
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The Distribution of Quiet Sun Magnetic Field Strengths from 0 to 1800 GThe quiet-Sun photospheric plasma has a variety of magnetic field strengths going from zero to 1800 G. The empirical characterization of these field strengths requires a probability density function (PDF), i.e., a function P(B) describing the fraction of quiet Sun occupied by each field strength B. We show how to combine magnetic field strengthDomínguez Cerdeña, I. et al.
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The color signature of the transit of HD 209458: discrepancies between stellar atmospheric models and observationsExoplanetary transits produce a double-horned color signature that is distinct from both binaries and blends and can thus be used to separate exoplanets from false positives in transit searches. Color photometry with precision sufficient to detect this signal in transits of HD 209458 is available in the literature. Analysis of these observationsTingley, B. et al.
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