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A Cool Supergiant with Anomalous Behavior of the 2800 MG II Doublet
Kondo, Y.; Gurzadian, G. A.; Rustambekian, S. S. +2 more
The IUE ultraviolet spectrum for a supergiant of type G Ia, HD 135345, is obtained for the wavelength region 2000-3000 A. In the spectrum, the continuum as well as the feature of the Mg II doublet at 2800 A is found to be anomalous. The observed level of continuum increases toward short wavelengths to 2000 A, verifying that this supergiant is actu…
Narrow Iron K-line and Warm Iron K-edge in Pulse Phase Spectra of Hercules X-1
Kahabka, Peter
Spectra of the accreting neutron star Hercules X-1 observed with the EXOSAT GSPC detector on days 61,65,92 and 96 1984 were analysed for iron line features. A broad gaussian emission line with a FWHM of 1.32±0.13 keV was found during on, turn-off and short-on states in the 35-day-cycle at an energy of ~ 6.55keV in the pulse phase averaged spectra.…
The reference frames in the data reduction of Hipparcos satellite.
Ling, Zhao-fen
Infrared and radio astronomy, and astrometry. Proceedings. Symposia 7, 8 and Topical Meeting of the COSPAR Interdisciplinary Scientific Commission E (Meeting E5) of the COSPAR 28. Plenary Meeting: Infrared and radio astronomy, and astrometry, The Hague (Netherlands), 25 Jun - 6 Jul 1990.
Perryman, M. A. C.; Smoot, G. F.; Wesselius, P. R. +2 more
Contents: 1. Astrometry from space (Symposium 7). 2. The infrared and submillimeter universe at high redshift (Symposium 8). 3. Space VLBI (Meeting E5).
Le nouvel astrolabe de l'Observatoire de Paris
Chollet, F.
The new polyvalent astrolabe of the Paris Observatory is described. After some optical modifications this new instrument is able to observe the stars, some planets, and the sun with an internal error less than 0.4 arcsec in the last case. Some new modifications are in progress to obtain better results and stability in the solar observations. This …
Ultraviolet Variability of the Massive W-R Binary System HDE 311884 = WR 47
Moffat, Anthony F. J.; Koenigsberger, Gloria; Auer, Lawrence H.
IUE observations and their analysis of the massive WN6 + O binary system HDE 311884 are presented. The phase-dependent variations are like those of WN4-6 binaries studied previously, with atmospheric eclipses evident in the N IV 1718 A and C IV 1550 A lines, and in the Fe V + VI pseudocontinuum at wavelengths below 1480 A. The considerable variabi…
Low-Resolution Spectra of Stellar Coronae and Flares with EXOSAT: The Iron K-line
Tagliaferri, G.; Pallavicini, R.
IUE Archival Spectra of 31 Cygni
Kang, Young Woon
UV light curve of 31 Cygni has been made from the IUE high dispersion spectra. The depth of primary minimum of the light curve is 5.2 magnitudes because the B4 star's steep spectral gradient. The light curve has been analyzed by the method of Wilson and Devinney Differential Correction(WD). The radial velocities have been measured using the Mg ¥± …
Residuals for the Observations of the 62 Selected Minor Planets
Calaf, J.
This paper reports results of the improvement of orbital elements of the 62 minor planets included in the Hipparcos mission. The astrometric observations supplied by the Minor Planet Center and the meridian circles at La Palma and Bordeaux observatories were used by the author. The accuracy reached (RMS O-C) for each minor planet and for La Palma …
Reexamination of discrete sources with ????b > 20 from COS-B data
Ma, Y.; Luo, Y.; Yu, K. N. +1 more
Using the cross-correlation and bootstrap sampling methods, the COS-B data in the observations with I b I > 20° are re-examined to search for discrete sources. Two source features have been identified and the possible counterparts are the pulsar PSR0950+08 and the weak