We have obtained I-, J-, H- and K-band light curves of the recurrent nova TCrB. We find that we can fit the J-band light curve only with a Roche lobe filling secondary star and a dark spot of radius 11 deg-26 deg (90 per cent confidence) centred at the inner Lagrangian point. We obtain limits to the binary inclination of 38 deg-46 deg (90 per cent

Line asymmetries and shifts are powerful tools for studying velocity fields in the stellar photospheres. Other effects, however, could also generate asymmetries, blurring the information of the velocity patterns. We have studied the shifts and asymmetries induced in the profiles of spectral lines by pressure effects. The best theoretical and

Even the most sensitive cosmic microwave background anisotropy experiments have signal-to-noise ratios

We present the first observational evidence for a collimated jet in a short-period cataclysmic variable system: the recurrent nova T Pyxidis. Optical spectra show bipolar components of H alpha with velocities ~1400 km s-1, very similar to those observed in the supersoft X-ray sources and in SS 433. We argue that a key ingredient of the formation of

In this paper we report CCD photometry in broad band B, R, and I colors, as well as in the Hα, for a sample of eight HII galaxies with strong radio emission. In addition, we present new radio continuum observations in the frequency range between 8 and 15GHz. For seven of these galaxies, previous radio continuum observations have been reported by

The Iris network for helioseismology has operated since 1989. We present tables of solar p-mode frequencies for observations taken during the four summer seasons from 1989 to 1992. This analysis uses the technique of maximum likelihood fitting and a χ_2_^2^ model for the probability density function of the spectrum. The simultaneous fitting of odd