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The observed shift of the core of the relativistic AGN jets as a function of frequency allows us to evaluate the number density of outflowing plasma and, hence, the magnetization parameter. New analys...
The possibility of distinguishing of scalar field models of dark energy with different Lagrangians and time variable equation of state parameter by available observational data is analyzed. The mul-ti...
We explore the precision with which the Einstein Telescope (ET) will be able to measure the parameters of intermediate–mass–ratio inspirals (IMRIs), i.e., the inspirals of stellar mass compact object...
Frequency separations used to infer global properties of stars through asteroseismology can change depending on the strength and at what epoch of the stellar cycle the p-mode frequencies are measured....
Fireball model of the gamma-ray bursts (GRBs) predicts generation of numerous internal shocks, which efficiently accelerate charged particles and generate relatively small-scale stochastic magnetic an...
We present two independent methods for studying the global stellar parameter space (mass M, age, chemical composition X0, Z0) of HD 49933 with seismic data. Using a local minimization and an MCMC algo...
This paper is a review on the observational Hubble parameter data that have gained increasing attention in recent years for their illuminating power on the dark side of the universe --- the dark matte...
The subject of this paper is an investigation of the nonlinear contributions to the spectrum of the integrated Sachs-Wolfe (iSW) effect. We derive the corrections to the iSW-auto spectrum and the iSW-...
Addendum: STARK BROADENING PARAMETER TABLES FOR Be I LINES OF ASTROPHYSICAL INTEREST。
STARK BROADENING PARAMETER TABLES FOR Ne VIII AND Na IX LINES OF ASTROPHYSICAL INTEREST。
STARK BROADENING PARAMETER TABLES FOR Al XI AND Si XII LINES OF ASTROPHYSICAL INTEREST。
Errata: STARK BROADENING PARAMETER TABLES FOR Mg I LINES OF INTEREST FOR SOLAR AND STELLAR SPECTRA RESEARCH I。

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