Deviations from a uniform period spacing of gravity modes in a massive star

A long-term spectroscopic and photometric survey of the most luminous and massive stars in the vicinity of the supermassive black hole Sgr A* revealed two new binaries: a

Subsequent analysis of B stars in the Small Magellanic Cloud (SMC) also re- vealed the presence of N-rich stars with low V sin i ( Hunter et al. The Galactic sample of B stars of

Association of Insulin-like Growth Factor 1 Concentrations with Risk for and Prognosis of Amyotrophic Lateral Sclerosis - Results from the ALS Registry Swabia... Association

Pour avoir un spectre de transmission du banc donnant une référence pour les futures mesures de transmission des composants, il faut que le montage à vide soit identique au montage

The second regime between 7 days to 8 months corresponds to the synoptic scales linked to the general circulation.The last alignment of points 16 to 18, which corresponds to

An exception was found for inhomogeneous clouds characterized by a small information codimension, a large cloud optical thickness, and a large single-scattering albedo and

During the period of effluent release, redox conditions are slightly suboxic in the upper 5 cm, with redox values higher than 200 mV, concentrations in dissolved Fe close to 25 µmol

We aim at deriving analytical prescriptions for period spacings of low-frequency gravity modes strongly affected by rotation through the full Coriolis acceleration (i.e.