137 citations · 795 across the 32 of their papers we have counts for
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ALMA observations of alpha Centauri: First detection of main-sequence stars at 3mm wavelength
R. Liseau, W. Vlemmings, A. Bayo +19
The precise mechanisms that provide the non-radiative energy for heating the chromosphere and the corona of the Sun and those of other stars constitute an active field of research.…
The Chromospheric Solar Millimeter-wave Cavity; a Common Property in the Semi-empirical Models
Victor De la Luz, Miguel Chavez, Emanuele Bertone
The semi-empirical models of the solar chromosphere are useful in the study of the solar radio emission at millimeter - infrared wavelengths. However, current models do not reprodu…
The FEROS--Lick/SDSS observational database of spectral indices of FGK stars for stellar population studies
M. Franchini, C. Morossi, P. Di Marcantonio +2
We present FEROS--Lick/SDSS, an empirical database of Lick/SDSS spectral indices of FGK stars to be used in population synthesis projects for discriminating different stellar popul…
The Limb Brightening and its Relationship with the Millimeter-wave Cavity
Victor De la Luz, Miguel Chavez, Emanuele Bertone
Through a detailed theoretical analysis of the local emission at millimeter,sub-millimeter and infrared wavelength regimes (from \~ 10 GHz up to \~ 10 THz), we found that, associat…
The Relation between the Radial Temperature Profile in the Chromosphere and the Solar Spectrum at Centimeter, Millimeter, Sub-millimeter, and Infrared Wavelengths
Victor De la Luz, Miguel Chavez, Emanuele Bertone +1
Solar observations from millimeter to ultraviolet wavelengths show that there is a temperature minimum between photosphere and chromosphere. Analysis based on semi-empirical models…