Misaligned spin-orbit in the XO-3 planetary system?
The transiting extrasolar planet XO-3b is remarkable, with a high mass and eccentric orbit. These unusual characteristics make it interesting to test whether...
Misleading variations in estimated rotational frequency splittings of solar p modes: consequences for helioseismology and asteroseismology
The aim of this paper is to investigate whether there are any 11-yr or quasi-biennial solar-cycle-related variations in solar rotational splitting frequencies...
Missing dust of super-early galaxies: Supernova blowout and gas─dust venting in blue monsters
Context. A subset of very young super-early galaxies at z ≳ 10, often called blue monsters, shows extremely blue UV continua and faint far-IR emission. This...
Missing large-angle correlations versus even-odd point-parity imbalance in the cosmic microwave background
Context. The existence of a maximum correlation angle (θ max ≳ 60°) in the two-point angular temperature correlations of cosmic microwave background (CMB)...
MIUSCAT: extended MILES spectral coverage - I. Stellar population synthesis models
We extend the spectral range of our stellar population synthesis models based on the MILES and CaT empirical stellar spectral libraries. For this purpose, we...
MIUSCAT: extended MILES spectral coverage - II. Constraints from optical photometry
In this work, we show a comprehensive comparison of our new stellar population synthesis (SPS) MIUSCAT models with photometric data of globular clusters (GCs)...
Mixed early and late-type properties in the bar of NGC 6221: Evidence for evolution along the Hubble sequence?
Rotation curves and velocity dispersion profiles are presented for both the stellar and gaseous components along five different position angles (PA =5(deg) , 50...
Mixed properties of MHD waves in non-uniform plasmas
This paper investigates the mixed properties of MHD waves in a non-uniform plasma. It starts with a short revision of MHD waves in a uniform plasma of infinite...
Mixing by internal waves. III. Li and Be abundance dependence on spectral type, age and rotation
In this paper we deal with the problem of the generation of internal waves at the bottom of convective zone in solar-type stars, and with the transport process...