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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Are magnetic fields shaping PNe?Not AvailableMatínez González, M. J. et al.
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42011 -
Activity indexes and velocities for 890 stars (Jenkins+, 2011)The activities, rotational velocities, radial velocities and kinematic space motions are presented for over 850 dwarf and subgiant FGK type stars. The chromospheric activities were measured using the CaII HK lines and high resolution and high S/N FEROS spectra. The radial velocities were determined by cross-correlation with a number of templateJenkins, J. S. et al.
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42011 -
Abundances of 650 bulge red giants (Gonzalez+, 2011)Listed are the [Mg/Fe], [Ca/Fe], [Ti/Fe] and [Si/Fe] abundance ratios for 650 K giants in four fields of the Galactic Bulge. Abundances were measured using standard 1D local thermodynamic equilibrium MARCS models and spectral synthesis using MOOG. The list also includes the metallicities [Fe/H] presented in Zoccali et al. (2008, Cat. J/A+A/486/177)Gonzalez, O. A. et al.
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42011 -
A Sounding Rocket Experiment for Spectropolarimetric Observations with the Lyα Line at 121.6 nm (CLASP)A team consisting of Japan, USA, Spain, and Norway is developing a high-throughput Chromospheric Lyman-Alpha SpectroPolarimeter (CLASP), which is proposed to fly with a NASA sounding rocket in 2014. CLASP will explore the magnetism of the upper solar chromosphere and transition region via the Hanle effect of the Lyα line for the first time. ThisIshikawa, R. et al.
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42011 -
VLT-VIMOS integral field spectroscopy of luminous and ultraluminous infrared galaxies. III. The atlas of the stellar and ionized gas distributionContext. Luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) are much more numerous at higher redshifts than locally, dominating the star-formation rate density at redshifts ~1-2. Therefore, they are important objects in order to understand how galaxies form and evolve through cosmic time. Local samples provide a unique opportunity toRodríguez-Zaurín, J. et al.
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