We report YALO consortium observation of a mini-outburst of Aquila X-1 = V1333 Aql, which occurred between July 04.27 and 07.29 UT. This X-ray binary outbursts approximately once per year, and most recently entered a mini-outburst during May 2000 (IAUC 7423,7429). We have been monitoring this source since April 5 in R using the YALO 1-m telescope

The study of the stellar content and physics of the ionized gas in local high-mass star-forming regions is specially important for better understanding extragalactic starbursts. Recent observations from space telescopes and near-infrared detectors have provided a wealth of new information about the gas and stars in these objects. In this paper, I

Realistic ab-initio 3D, radiative-hydrodynamical convection simulations of the solar granulation have been applied to Fe i and Fe ii line formation. In contrast to classical analyses based on hydrostatic 1D model atmospheres the procedure contains no adjustable free parameters but the treatment of the numerical viscosity in the construction of the

We limit the contribution of the hot intracluster gas, by means of the Sunyaev-Zeldovich effect, to the temperature anisotropies measured by the Tenerife experiment. The data are cross-correlated with maps generated from the ACO cluster catalog, the ROSAT PSPC catalog of clusters of galaxies, a catalog of superclusters and the HEAO 1 A-1 map of X

Various radial velocity surveys have now produced a number of candidates Very Low Mass Stars, Brown Dwarfs and Giant Extrasolar Planets to nearby G, K and M dwarfs. Building upon our experience in High Angular Resolution imaging, radial velocities measurements and atmosphere modeling, we discuss the detectability of Brown Dwarfs and Extrasolar

We have obtained NIR broad-band images in the J, H and K bands of 12 barred galaxies that make up our sample, during three observing runs with the 3.6 m Canada-France-Hawaii Telescope on Hawaii. We used the Montreal NIR camera (MONICA) equipped with a 256 x 256 pixel HgCdTe array detector with a projected size of 0.248 arcsec. One of the main data