We report optical spectroscopy and redshift determination for 22 radio galaxies, extracted from the Ekers et al. (1989) compilation. Selected sources, which...
Redshift-distance relations from type Ia supernova observations. New constraints on grey dust models
Extinction due to intergalactic grey dust has been proposed as an alternative to accelerated expansion to account for the dimming of SnIa fluxes beyond z ≃ 0.5...
Reduced atomic models for large-scale computations: Fe XIII near-infrared lines
Accurate atomic models for astrophysical plasma can be very complex, requiring thousands of states. However, for a variety of applications such as large-scale...
Reduction of asteroidal appulses. First results in Bucharest
The method presented is applied to asteroidal approaches to catalogue stars and occultations, and derives the minimum separation at conjunction and the...
Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction
In 1981, the idea of a superwind that ends the life of cool giant stars was proposed1. Extreme oxygen-rich giants, OH/IR stars, develop superwinds with the...
Refined Orbital Solution and Quiescent Variability in the Black Hole Transient GS 1354-64 (= BW Cir)
In Casares et al. we presented the first radial velocity curve of the companion star to BW Cir which demonstrates the presence of a black hole in this...
Refined parameters of the HD 22946 planetary system and the true orbital period of planet d★
Context. Multi-planet systems are important sources of information regarding the evolution of planets. However, the long-period planets in these systems often...
Refinements to the Solar Polar Magnetic Flux: Implications from Inversion Methodologies
The magnetic fields in the solar polar region are important to our understanding of the internal dynamo process, the global coronal structure, and the origin of...