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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Massive star formation in Wolf-Rayet galaxies. V. Star-formation rates, masses and the importance of galaxy interactionsAims: We performed a comprehensive analysis of a sample of 20 starburst galaxies that show a substantial population of very young massive stars, most of them classified as Wolf-Rayet galaxies. Methods: In this paper, the last in the series, we analyze the global properties of our galaxy sample using multiwavelength data extracted from our ownLópez-Sánchez, Á. R.
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102010 -
Magnetic fields and the outer rotation curve of M31Not AvailableRuiz-Granados, B., et al.
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102010 -
MAGIC Telescope Observations of Gamma-Ray BurstsMAGIC is built to perform observations of prompt and early afterglow emission from Gamma-Ray Bursts (GRBs) above 25 GeV. The instrument is designed to have the lowest possible energy threshold among the ground based γ-ray detectors and the fastest reaction time to alerts distributed over the GRB Coordinates Network (GCN). The MAGIC-I telescopeGarczarczyk, M. et al.
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102010 -
Long-term Evolution of the Aerosol Debris Cloud Produced by the 2009 Impact of an Object with JupiterWe report the evolution of the cloud of aerosols produced in the atmosphere of Jupiter by the impact of an object in 19 July 2009 (Sánchez-Lavega et al., Astrophys. J. Lett, Vol. 715, L155. 2010). This study is based on images obtained with a battery of ground-based telescopes and the Hubble Space Telescope in the visible and in the deep nearSanchez-Lavega, Agustin et al.
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102010 -
Limits on the orbits and masses of moons around currently-known transiting exoplanetsAims: Current and upcoming space missions may be able to detect moons of transiting extra-solar planets. In this context it is important to understand if exomoons are expected to exist and what their possible properties are. Methods: Using estimates for the stability of exomoon orbits from numerical studies, a list of 87 known transiting exoplanetsWeidner, C. et al.
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102010