The temporal and spatial behaviour of the K I 769.9 nm solar line are investigated using several series of high spectral resolution low-noise photoelectric scans obtained at Kitt Peak National Observatory in quiet and active (plages and sunspots) regions. Corrections due to the instrumental profile were applied to yield the best line shape. A

IAUC 4613 available at Central Bureau for Astronomical Telegrams. IAUC 4613 available at Central Bureau for Astronomical Telegrams.

The authors present the results of a near-infrared survey of 13 areas containing 16 GGD objects. A total of 12 infrared sources have been detected in five of the surveyed fields; six of them are new detections. An IRAS point source is present in all the areas where the authors have positive detections. The infrared colours J-H, H-K and K-L indicate

A new technique to calculate multilevel non-LTE continuum formation in the UV of stellar winds and plane-parallel, static stellar atmospheres is developed using a local approximate lambda operator similar to those presented by Werner and Husfeld (1985) and Hamann (1986). In the present formulation, the iteration of the transfer equation solution is

The ESO 32-channel infrared (1 -5 micron-meter) grating spectrometer, IRSPEC, was put into operation and made available for Visiting Astronomers in October 1986. In this contribution we describe the reduction scheme implemented in MIDAS to process IRSPEC data taken in any of the two - discrete or Continuous - instrumental modes. The Ins~rument

An attempt is made to explain conflicting experimental data recently obtained concerning the frequency stability of solar oscillations. Extensive data obtained at the Observatorio del Teide are analyzed to determine the lifetimes and frequencies of the l0 and l1 p-modes. The importance of the lifetime of the mode in determining the frequency is