Search Publications

KDG218, a nearby ultra-diffuse galaxy
DOI: 10.1134/S1990341317040022 Bibcode: 2017AstBu..72..376K

Sharina, M. E.; Karachentsev, I. D.; Makarova, L. N. +1 more

We present properties of the low-surface-brightness galaxy KDG218 observed with the HST/ACS. The galaxy has a half-light (effective) diameter of ae = 47″ and a central surface brightness of SBV(0) = 24.m4/□″. The galaxy remains unresolved with the HST/ACS, which implies its distance of D > 13.1 Mpc and linear ef…

2017 Astrophysical Bulletin
eHST 12
IR photometry results and dust envelope model for symbiotic Mira star candidate V 335 Vul
DOI: 10.1134/S1990341317040071 Bibcode: 2017AstBu..72..447B

Bogdanov, M. B.; Taranova, O. G.; Shenavrin, V. I.

We present the results of JHKLM-photometry for the symbiotic Mira star candidate V 335 Vul. Based on the average flux data, supplemented by IRAS, MSX, AKARI, and WISE mid-IR observations, we calculated a model of a spherically symmetric dust envelope of the star, made up of amorphous carbon and silicon carbide particles. The optical depth of the e…

2017 Astrophysical Bulletin
AKARI 0
A comparison of properties of different population radio galaxies based on the Planck mission microwave data
DOI: 10.1134/S1990341316020024 Bibcode: 2016AstBu..71..139V

Verkhodanov, O. V.; Solovyov, D. I.; Khabibullina, M. L. +1 more

Applying the stacking method, we examine the areas of the cosmic microwave background radiation (CMB) maps, constructed according to the Planck SpaceObservatory data in the neighbourhood of different populations of radio sources and giant elliptical galaxies. The samples of objects include giant radio galaxies (GRG), radio sources, selected by the…

2016 Astrophysical Bulletin
Planck 11
A comparison of anisotropic statistical properties of CMB maps based on the WMAP and planck space mission data
DOI: 10.1134/S1990341316040015 Bibcode: 2016AstBu..71..371V

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

We compare the anisotropic properties of the cosmic microwave background (CMB) maps constructed based on the data of NASA's WMAP (9th year of observations) and ESA's Planck (2015 release) space missions. In our analysis, we use two two-dimensional estimators of the scatter of the signal on a sphere, which amount to algorithms of mapping the ratio …

2016 Astrophysical Bulletin
Planck 1
Investigation of the RCR catalog sources in the millimeter and submillimeter ranges based on the Planck mission data
DOI: 10.1134/S1990341315020030 Bibcode: 2015AstBu..70..156V

Verkhodanov, O. V.; Majorova, E. K.; Zhelenkova, O. P. +3 more

We have studied the regions of the microwave background radiation maps of the Planck experiment in the neighborhood of the RCR catalog radio sources. From the processed data for bright radio sources in the microwave range, we plotted the calibration curves which allow the brightness of the objects to be measured. For the first time, for 117 object…

2015 Astrophysical Bulletin
Planck 15
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
Speckle interferometry of nearby multiple stars. V. 2002–2006 positional measurements
DOI: 10.1134/S1990341313010057 Bibcode: 2013AstBu..68...53B

Dyachenko, V. V.; Rastegaev, D. A.; Balega, Yu. Yu. +5 more

We present the measurements of positional parameters of 194 nearby binary stars performed at the 6-m BTA telescope of the SAO RAS from 2002 through 2006 applying the speckle interferometric technique. The observations were conducted at central filter wavelengths ranging from 545 to 800 nm using a speckle interferometer equipped with a fast CCD and…

2013 Astrophysical Bulletin
Hipparcos 38