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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Mediterranean Archaeotopography and Archaeoastronomy: Two Examples of Dolmenic Necropolises in the Jordan ValleyNot AvailableBelmonte, J. A.
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1997 -
Violent Star Formation in NGC 2363: ErratumIn the paper "Violent Star Formation in NGC 2363" by Rosa M. Gonzalez- Delgado, Enrique Perez, Guillermo Tenorio-Tagle, Jose M. Vilchez, Elena Terlevich, Roberto Terlevich, Eduardo Telles, Jose M. Rodriguez-Espinosa, Miguel Mas-Hesse, Maria Luisa Garcia-Vargas, Angeles I. Diaz, Jordi Cepa, and Hector Castaneda (ApJ, 437,239 [1994)), there are threeGonzalez-Delgado, Rosa M. et al.
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121996 -
The Stromgren Transition as a Diagnostic for Massive Star FormationIn the luminosity functions (LF's) of the HII regions of a set of late-type spiral galaxies we have identified the presence of a phase-change via a jump in the function accompanied by a change in slope.The nature of the phase-change is diagnosed using measurements of the internal radial surface brightness of individual regions.Plotting the internalBeckman, J. E. et al.
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121996 -
The magnetic structure of pores and sunspots derived from Advanced Stokes Polarimeter data.We investigate the radial variation of the magnetic field structure across sunspots, pores and azimuth centers (ACs). We define ACs as magnetic structures of about the same size as pores (all structures studied here are larger than 3 Mm diameter), but without a clear (at least 5%) continuum decrease associated with them. We start from the full 3DKeppens, R. et al.
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121996 -
The Local Group Dwarf Irregular Galaxy NGC 6822.III. The Recent Star Formation HistoryWe present a quantitative derivation of the recent star formation history (SFH) in different regions in the main body of NGC 6822. It has been performed using a set of model CM diagrams computed under different assumptions for the recent (~400 Myr) SFH and in which the crowding effects have been simulated using the particular crowding informationGallart, C. et al.
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121996