Search Publications
A study of the radial velocity of the star theta 1 Ori C.
Vitrichenko, E. A.
A Chemically Decoupled Nucleus and Inner Polar Ring of the SBb Galaxy NGC 4548
Sil'chenko, O. K.
A Preliminary Radial-Velocity Curve for the Star θ1 Ori D
Vitrichenko, É. A.
Astrometric Orbits from a Direct Combination of Ground-Based Catalogs with the Hipparcos Catalog
Kiyaeva, O. V.; Goncharov, G. A.
Analysis of HST Ultraviolet Spectra for T Tauri Stars: Estimating the Interstellar Extinction and the Contribution from an Accretion Shock to the Emission-Continuum Formation
Lamzin, S. A.; Kravtsova, A. S.
Acoustic Power Mapping for Active Regions from MDI, HLH, and TON Data
Hill, F.; Ladenkov, O. V.; Egamberdiev, Sh. A. +1 more
Two-Dimensional Spectroscopy of Double-Barred Galaxies
Moiseev, A. V.
We describe the results of our spectroscopy for a sample of barred galaxies whose inner regions exhibit an isophotal twist commonly called a secondary bar. The line-of-sight velocity fields of the ionized gas and stars and the light-of-sight velocity dispersion fields of the stars were constructed from two-dimensional spectroscopy with the 6m Spec…
A minimum in the light curve of the classical symbiotic star YY Her in 2001.
Kolotilov, E. A.; Yudin, B. F.; Tatarnikova, A. A. +1 more
Trigonometric Parallaxes and a Kinematically Adjusted Distance Scale for OB Associations
Dambis, A. K.; Rastorguev, A. S.; Mel'Nik, A. M.
By directly comparing the photometric distances of Blaha and Humphreys (1989) (BH) to OB associations and field stars with the corresponding Hipparcos trigonometric parallaxes, we show that the BH distance scale is overestimated, on average, by 10-20%. This result is independently corroborated by applying the rigorous statistical-parallax method a…
An Astrometric Study of the Triple Star ADS 48
Kiselev, A. A.; Kiyaeva, O. V.; Polyakov, E. V. +1 more
We analyze the series of relative positions of the hierarchical triple system ADS 48 ABF (AB = 6 arcsec, AF = 327 arcsec) obtained with the 26-inch Pulkovo refractor during 1961-1995 and measured with the Fantazia automated measuring system. A new relative orbit of pair AB is determined by the method of apparent-motion parameters using new observa…