Context. Blue compact galaxies (BCG) are narrow emission-line systems that undergo a violent burst of star formation. They are compact, low-luminosity galaxies, with blue colors and low chemical abundances, which offer us a unique opportunity to investigate collective star formation and its effects on galaxy evolution in a relatively simple
Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..
Además ofrece acceso al repositorio de preprints del IAC: https://research.iac.es/preprints/l
-
Mapping luminous blue compact galaxies with VIRUS-P. Morphology, line ratios, and kinematicsCairós, L. M. et al.112012
-
Mapping the Sky at Centimetric Wavelengths with Circular Scans
We have constructed an instrument able to map the sky at 10 GHz using circular scans with an angular resolution of 1deg. This instrument consist of a spinning plate working as a primary mirror for a parabolic dish with two cryogenic receptors at its focus. The area observed is a band of 20deg in Dec and the full sky in RA, centered at Dec 28 (the
Gallegos, J. et al.Fecha de publicación:
111998 -
Marking the 400th Anniversary of Kepler's Astronomia nova
Special Session 9 of the XXVII General Assembly (11-14 August 2009, Rio de Janeiro) was devoted to the topic “Marking the 400th Anniversary of Kepler's Astronomia nova”. During the two-and-a-half day meeting (spread over four days), there were nine invited and three contributed talks, a round-table discussion on the future of Kepler studies and an
Mahoney, T. J.Fecha de publicación:
112010 -
MARS: The MAGIC Analysis and Reconstruction Software
With the commissioning of the second MAGIC gamma-ray Cherenkov telescope situated close to MAGIC-I, the standard analysis package of the MAGIC collaboration, MARS, has been upgraded in order to perform the stereoscopic reconstruction of the detected atmospheric showers. MARS is a ROOT-based code written in C++, which includes all the necessary
Moralejo, R. A. et al.Fecha de publicación:
112010 -
MASGOMAS project: building a bona-fide catalog of massive star cluster candidates
MASGOMAS (MAssive Stars in Galactic Obscured MAssive clusterS) is a project aiming at discovering OB stars in Galactic, dust enshrouded, star-forming massive clusters (Marín-Franch et al. 2009, A&A 502, 559). The project has gone through different phases of increasing automatization, that have allowed us to discover massive clusters like MASGOMAS-1
Herrero, A. et al.Fecha de publicación:
112017 -
Mass, metallicity and SFR relationships in star forming galaxies using deep surveys
Not Available
Lara-Lopez, M. A.Fecha de publicación:
112011