Modulation of Circumstellar Extinction in a Young Binary System with a Low-Mass Companion in a Noncoplanar Orbit

The cyclic activity model of a young star with the low-mass secondary component (q = M2/M1 <= 0.1) accreting a matter from circumbinary disk is considered. It is assumed that the orbit is circular and the disk and orbital planes are non-coplanar. Sets of hydrodynamics models of such a system have been calculated by the SPH method and then the variations of the circumstellar extinction and phase light curves were determined. The calculations showed that depending on the model parameters and orientation of the system in regards to an observer the different in shape and amplitude light curves can be observed. An important property of the considered models is also the dependence of the mass accretion rate onto the components on the phase of the orbital period. The results of the calculation can be used for analysis of the cyclic activity of UX Ori stars and young stars with the long-lasting eclipses.Comment: 14 pages, 7 figure

Estimating the Dark Halo Mass from the Relative Thickness of Stellar Disks

We analyze the relationship between the mass of a spherical component and the minimum possible thickness of stable stellar disks. This relationship for real galaxies allows the lower limit on the dark halo mass to be estimated (the thinner the stable stellar disk is, the more massive the dark halo must be). In our analysis, we use both theoretical relations and numerical N-body simulations of the dynamical evolution of thin disks in the presence of spherical components with different density profiles and different masses. We conclude that the theoretical relationship between the thickness of disk galaxies and the mass of their spherical components is a lower envelope for the model data points. We recommend using this theoretical relationship to estimate the lower limit for the dark halo mass in galaxies. The estimate obtained turns out to be weak. Even for the thinnest galaxies, the dark halo mass within four exponential disk scale lengths must be more than one stellar disk mass.Comment: 20 pages including 6 figures. To be published in Astronomy Letters (v. 32, No. 10, pp. 649-660, 2006

Hydrodynamic Processes in Young Binary Systems as a Source of Cyclic Variations of Circumstellar Extinction

Hydrodynamic models of a young binary system accreting matter from the remnants of a protostellar cloud have been calculated by the SPH method. It is shown that periodic variations in column density in projection onto the primary component take place at low inclinations of the binary plane to the line of sight. They can result in periodic extinction variations. Three periodic components can exist in general case. The first component has a period equal to the orbital one and is attributable to the streams of matter penetrating into the inner regions of the binary. The second component has a period that is a factor of 5-8 longer than the orbital one and is related to the density waves generated in a circumbinary (CB) disk. The third, longest period is attributable to the precession of the inner asymmetric region of CB disk. The relationship between the amplitudes of these cycles depends on the model parameters as well as on the inclination and orientation of the binary in space. We show that at a dust-to-gas ratio of 1:100 and and a mass extinction coefficient of 250 cm$^2$ g$^{-1}$, the amplitude of the brightness variations of the primary component in the V-band can reach $1^m$ at a mass accretion rate onto the binary components of $10^{-8} M_{\odot}$ yr$^{-1}$ and a $10^{\rm o}$ inclination of the binary plane to the line of sight. We discuss possible applications of the model to pre-main-sequence stars.Comment: 13 pages, 6 figures, published in Astronomy Letters (v.33, 2007

New insights from old cosmic rays: A novel analysis of archival KASCADE data

Cosmic ray data collected by the KASCADE air shower experiment are competitive in terms of quality and statistics with those of modern observatories. We present a novel mass composition analysis based on archival data acquired from 1998 to 2013 provided by the KASCADE Cosmic ray Data Center (KCDC). The analysis is based on modern machine learning techniques trained on simulation data provided by KCDC. We present spectra for individual groups of primary nuclei, the results of a search for anisotropies in the event arrival directions taking mass composition into account, and search for gamma-ray candidates in the PeV energy domain.Comment: Proceedings of the 37th International Cosmic Ray Conference (ICRC2021), 12-23 July 2021, Berlin, Germany - Onlin

Environmental monitoring of natural waters in Krasnodar and Stavropol Territories

The environmental monitoring of natural waters in Krasnodar (Uspensky and Novokubansky districts) and Stavropol (Kochubeyevsky District) Territories was conducted. In the course of study, various elements and compounds harmful to animals and humans, which exceed maximum permissible concentrations, were identified

Radio properties of high-redshift galaxies at z≥1z \geq 1

Study of high-redshift radio galaxies (HzRGs) can shed light on the active galactic nuclei (AGNs) evolution in massive elliptical galaxies. The vast majority of observed high-redshift AGNs are quasars, and there are very few radio galaxies at redshifts $z>3$. We present the radio properties of 173 sources optically identified with radio galaxies at $z\geqslant1$ with flux densities $S_{1.4}\geqslant20$ mJy. Literature data were collected for compilation of broadband radio spectra, estimation of radio variability, radio luminosity, and radio loudness. Almost 60% of the galaxies have steep or ultra-steep radio spectra; 22% have flat, inverted, upturn, and complex spectral shapes, and 18% have peaked spectra (PS). The majority of the PS sources in the sample (20/31) are megahertz-peaked spectrum sources candidates, i.e. possibly very young and compact radio galaxies. The median values of the variability indices at 11 and 5 GHz are $V_{S_{11}}=0.14$ and $V_{S_{5}}=0.13$, which generally indicates a weak or moderate character of the long-term variability of the studied galaxies. The typical radio luminosity and radio loudness are $L_{5}=10^{43}$ - $10^{44}$ erg*s$^{-1}$ and $\log R=3$ - $4$ respectively. We have found less prominent features of the bright compact radio cores for our sample compared to high-redshift quasars at $z\geq3$. The variety of the obtained radio properties shows the different conditions for the formation of radio emission sources in galaxies

37 GHz observations of narrow-line Seyfert 1 galaxies

Observations at 37 GHz, performed at Mets\"ahovi Radio Observatory, are presented for a sample of 78 radio-loud and radio-quiet narrow-line Seyfert 1 (NLS1) galaxies, together with additional lower and higher frequency radio data from RATAN-600, Owens Valley Radio Observatory, and the Planck satellite. Most of the data have been gathered between February 2012 and April 2015 but for some sources even longer lightcurves exist. The detection rate at 37 GHz is around 19%, comparable to other populations of active galactic nuclei presumed to be faint at radio frequencies, such as BL Lac objects. Variability and spectral indices are determined for sources with enough detections. Based on the radio data, many NLS1 galaxies show a blazar-like radio spectra exhibiting significant variability. The spectra at a given time are often inverted or convex. The source of the high-frequency radio emission in NLS1 galaxies, detected at 37 GHz, is most probably a relativistic jet rather than star formation. Jets in NLS1 galaxies are therefore expected to be a much more common phenomenon than earlier assumed.Comment: Accepted for publication in A&A. Table of 37 GHz data will be available at the CDS soo

Mixed Morphology Pairs as a Breeding Ground for Active Nuclei

Mixed morphology pairs offer a simplification of the interaction equation that involves a gas-rich fast rotator paired with a gas-poor slow rotator. In past low resolution IRAS studies it was assumed that the bulk of the far infrared emission originated in the spiral component. However our ISO studies revealed a surprising number of early-type components with significant IR emission some of which turned out to show active nuclei. This motivated us to look at the current statistics of active nuclei in mixed pairs using the FIR-radio continuum correlation as a diagnostic. We find a clear excess of early-type components with radio continuum emission and an active nucleus. We suggest that they arise more often in mixed pairs via cross fueling of gas from the spiral companion. This fuel is more efficiently channeled into the nucleus of the slow rotating receptor. In a sample of 112 mixed-morphology pairs from the Karachentsev catalog we find that about 25-30% of detected mixed pairs show a displacement from the radio-FIR relation defined by normal star forming galaxies. The latter objects show excess radio continuum emission while others extend the relation to unusually high radio and FIR flux levels. Many of the outliers/extreme emitters involve an early-type component with an active nucleus. The paired E/S0 galaxies in the sample exhibit a significant excess detection fraction and a marginal excess luminosity distribution compared to isolated unpaired E/S0 galaxies.Comment: 3 figure

Закупка научного оборудования из средств грантов для центров коллективного пользования и уникальных научных установок

This study is devoted to identifying typical problems in the field of scientific equipment procurement in the interests of core shared research facilities and large-scale research facilities and developing approaches to their solution. The paper provides an analysis on the practice of purchasing scientific equipment, conducted on the basis of statistical data obtained from representatives of core shared research facilities and large-scale research facilities that received governmental support in 2019–2021, as well as on the data of a sociological survey. As a result, the hypotheses put forward by the authors about the predominance of foreign-made scientific equipment in the procurement structure, about the decrease in the average cost of purchased equipment in 2019–2021, about the presence of significant unevenness of scientific equipment by subclasses in the procurement structure of scientific equipment, about the presence of similar organizational problems in the field of procurement of scientific equipment. The article suggests a number of approaches to solving the identified problems arising from the formulations of 4 proven hypotheses.Настоящее исследование посвящено выявлению типовых проблем в области организации закупок научного оборудования в интересах центров коллективного пользования и уникальных научных установок, и разработке подходов к их решению. В работе дается анализ практики закупки научного оборудования, проведенный на основе статистических данных, полученных от представителей центров коллективного пользования и уникальных научных установок, получивших государственную поддержку в 2019–2021 гг., а также на данных социологического опроса. В результате нашли свое подтверждение выдвинутые авторами гипотезы о преобладании в структуре закупок научного оборудования иностранного производства, снижении средней стоимости закупленного оборудования в 2019–2021 гг., наличии значимой неравномерности по подклассам научного оборудования в структуре закупок научного оборудования, наличии однотипных проблем организационного характера в области организации закупок научного оборудования. В статье предложен ряд подходов к решению выявленных проблем, вытекающих из формулировок 4 доказанных гипотез

The Polar Stellar Ring and Dark Halo of NGC 5907

Numerical simulations of the disruption of a dwarf companion moving in the polar plane of a massive galaxy are presented. The constructed model is compared with observational data on the recently discovered low-surface-brightness stellar ring around galaxy NGC 5907. Constraints on the ring lifetime (<=1.5 gyr after the first approach of the galaxies), on the structure of companion -- the ring presecursor, and on mass of dark halo of the main galaxy in whose gravitational field the companion moves are provided. The dark halo mass within 50 kpc of NGC 5907 center cannot exceed 3 or 4 "visible" masses.Comment: 8 pages, 6 figures, article published in Astronomy Letters, Vol.26, No.5, 2000, pp277-28