Deep spectra of the planetary nebula IC 418 were obtained in the wavelength range 4190-5850 A. The data made it possible to map an extended halo about the...
The Coronae of AB Doradus and V471 Tauri: Primordial Angular Momentum versus Tidal Spin-up
The zero-age main-sequence star AB Dor and the K dwarf component of the V471 Tau close binary have essentially identical rotation rates and spectral types. An...
The Coronal Power Spectrum from MHD Mode Conversion above Sunspots
Sunspots are intense regions of magnetic flux that are rooted deep below the photosphere. It is well established that sunspots host magnetohydrodynamic waves...
The CoRoT ground-based asteroseismological programme
A large ground-based spectroscopic and photometric programme has accompanied the asteroseismological photometric observations of the satellite CoRoT since its...
The CoRoT target HD 175726: an active star with weak solar-like oscillations
Context: The CoRoT short runs give us the opportunity to observe a large variety of late-type stars through their solar-like oscillations. We report...
The CoRoT-7 planetary system: two orbiting super-Earths
We report on an intensive observational campaign carried out with HARPS at the 3.6 m telescope at La Silla on the star CoRoT-7. Additional simultaneous...
The Correlation between Mixing Length and Metallicity on the Giant Branch: Implications for Ages in the Gaia Era
In the updated APOGEE-Kepler catalog, we have asteroseismic and spectroscopic data for over 3000 first ascent red giants. Given the size and accuracy of this...
The correlation between photometric variability and radial velocity jitter. Based on TESS and HARPS observations
Context. Characterizing the relation between stellar photometric variability and radial velocity (RV) jitter can help us to better understand the physics behind...
The correlation structure of dark matter halo properties
We investigate the correlation between nine different dark matter halo properties using a rank correlation analysis and a Principal Component Analysis for a...