Search Publications

On discovery of strong magnetic field in the binary system HD34736
DOI: 10.1134/S1990341314020060 Bibcode: 2014AstBu..69..191S

Romanyuk, I. I.; Semenko, E. A.; Yakunin, I. A. +1 more

We present the results of a study of the star HD34736. The spectropolarimetric observations carried out at the 6-m telescope showed the presence of a strong variable longitudinal magnetic field, exceeding ‑4500 G. The analysis of the Hipparcos photometry gives a set of possible periods of the brightness variability of the star, of which

2014 Astrophysical Bulletin
Hipparcos 27
Physical and geometrical parameters of the binary system gliese 150.2
DOI: 10.1134/S1990341314020072 Bibcode: 2014AstBu..69..198A

Al-Wardat, M. A.; Balega, Yu. Yu.; Leushin, V. V. +4 more

The speckle interferometric binary system Gl 150.2 (HIP17491) is analyzed using atmosphere modeling and dynamical analysis simultaneously. A synthetic spectral energy distribution (SED) for each of the two components of the system is built using Kurucz blanketed models. These SEDs are combined together to form the total flux, which is compared wit…

2014 Astrophysical Bulletin
Hipparcos 18
Comparison of low-harmonics spectra and maps according to the WMAP and Planck space missions
DOI: 10.1134/S1990341314030092 Bibcode: 2014AstBu..69..330V

Verkhodanov, O. V.

We present a comparison of the angular power spectra and maps represented by the WMAP and Planck mission teams. The spectra are compared in the the multi pole range (2 ≤ ℓ ≤ 50). The ℓ =5, 7, 13, 29, 37, 41–46 harmonics have a discrepancy in the angular power spectra. The maps of the microwave background and their phase characteristics are studied…

2014 Astrophysical Bulletin
Planck 6
Two-dimensional spectral estimators of statistical anisotropy and search for the isolated directions in Planck mission data
DOI: 10.1134/S1990341314040105 Bibcode: 2014AstBu..69..488N

Verkhodanov, O. V.; Naiden, Ya. V.

We describe a method for the analysis of homogeneity of the microwave background maps based on the behavior of the angular power spectrum C(ℓ) and parity parameter P. The estimator is built using the dispersion variation of the power spectrum of the background signal hemisphere and allows to visualize the statistical anisotropy as a new map which …

2014 Astrophysical Bulletin
Planck 3