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Stark broadening of O VII and Mg XI
Using a semiclassical perturbation approach, we have calculated electron-, proton-, and He III-impact line widths and shifts for 14 O VII and 18 Mg XI multiplets. For O VII,... -
Einstein A-Coefficients in SiC2 transitions
Einstein A-coefficients for the electric dipole transitions in Silicon Dicarbide molecule and its isotopomers between rotational levels of the ground vibrational state up to... -
Astrometry of Satellites of Uranus
Table7 contains standard Co-ordinates (J2000.0) in arcseconds relative to the reference satellite. The numbers of the satellites 1-5 correspond to the conventional designation... -
Co II oscillator strengths
In table 2 the log(gf) values for the 3d^8^+3d^7^ 4s-->3d^7^ 4p electric dipole (E1) transitions are given. This system is selected by cutting off energy values larger than... -
Stark broadening of Na X
Using a semiclassical perturbation approach, we have calculated electron-, proton-, and He III-impact line widths and shifts for 57 Na X multiplets for perturber densities... -
WATCH Solar X-Ray Burst Catalogue
Catalogue containing solar X-ray bursts measured by the Danish Wide Angle Telescope for Cosmic Hard X-Rays (WATCH) experiment aboard the Russian satellite GRANAT in the deca-keV... -
Hipparcos intermediate astrometric data
Summary of the great circle statistics for FAST and NDAC reduction results, allowing the distinction of great circles according to the number of accepted single star transits. -
Double stars micrometer measurements
These tables report 458 micrometer observations of visual double stars made with the 152cm. telescope at Calar Alto Observatory (Almeria, Spain) and with the 35cm. telescope at... -
High-nl Rydberg states in C II, C III and C IV
Predicted term energies for values of the principal quantum number up to 30 and orbital quantum numbers l>=3 in C II, C III and C IV have been obtained using the Ritz and the... -
Si XI & Si XIII lines Stark broadening
Using a semiclassical perturbation approach, we have calculated electron-, proton-, and He III-impact line widths and shifts for 4 Si XI multiplets for perturber densities... -
Co II radiative transition probabilities
Radiative transition probabilities have been calculated for the magnetic dipole (M1) and electric quadrupole (E2) transitions connecting the 47 metastable energy levels in the... -
Proper motion LTT stars -5<DE<-30, 0<RA<13h30
Data are given for 353 LTT stars found on 42 areas, covering 25 square degrees each, with declination between -5{deg} and -30{deg} and right ascension between 0h and 13h 30m.... -
Vacuum ultraviolet emission band systems of N2
Observed wavenumbers of the emission lines belonging to 10 vacuum ultraviolet band systems of molecular nitrogen are classified into 283 bands, 220 of them reported for the... -
Stark broadening of Ca IX and Ca X lines
Using a semiclassical approach, we have calculated electron-, proton-, and He III-impact line widths and shifts for 4 Ca IX multiplets for perturber densities... -
X-ray Sources in Molecular Clouds
Figure 9: Finding charts for the objects where spectra were taken, based on the APM data base. The cross is centered at the X-ray position. 30 arcsec radius error circles are... -
Stark broadening of Kr II lines
With the development of space-borne spectroscopy, spectral line parameters for a large number of lines become of increasing interest for astrophysics. To provide Stark... -
Giants and supergiants ROSAT data
We present X-ray data for all late-type (A,F,G,K,M) giants and supergiants (luminosity classes I to III-IV) listed in the Bright Star Catalogue that have been detected in the... -
IRON Project XXVII. Fe IV collision strengths
Collision strengths and maxwellian-averaged rate coefficients have been calculated for 8771 non-vanishing transitions among 140 fine structure levels, dominated by the... -
Terzan 10, ESO456-SC38 and UKS 1 VIz photometry
We present optical colour-magnitude diagrams for the faint bulge globular clusters Terzan 10, ESO456-SC38 and UKS 1. The giant branches are detected but the horizontal branch is... -
Nice double star measurements
We present the last observations from two lists: General program and MLR pairs, made with the 50cm refractor of Nice Observatory.