405 research outputs found
Cobalt(II) and copper(II) complexes with carboxylic acids, imidazole, and 2-methylimidazole
The compositions of [MIm(MeIm)x]L complexes synthesized by the reaction of cobalt(II) and copper(II) fumarates ML Β· nH2O with imidazole (Im) and 2-methylimidazole (MeIm) were determined. The thermal decomposition of the salts was analyzed, and the pyridine nitrogen atom of imidazole and the oxygen atoms of carboxyl anions were shown to participate in complexation using electronic absorption spectra and IR spectra. The composition and stability of cobalt(II) and copper(II) imidazolatesuccinate complexes in an aqueous solution were determined photometrically and spectrophotometrically, and their higher stability in comparison with monoligand complexes was demonstrated
ΠΠΎΠ»ΡΡΠ΅Π½ΠΈΠ΅ Π½ΠΈΠ·ΠΊΠΎΠ·Π°ΡΡΡΠ²Π°ΡΡΠ΅Π³ΠΎ Π΄ΠΈΠ·Π΅Π»ΡΠ½ΠΎΠ³ΠΎ ΡΠΎΠΏΠ»ΠΈΠ²Π° Π΄Π»Ρ Π½Π°Π΄ΡΠΆΠ½ΠΎΠΉ ΡΠ°Π±ΠΎΡΡ ΡΠ΅Ρ Π½ΠΈΠΊΠΈ Π² ΡΠ°ΠΉΠΎΠ½Π°Ρ ΠΡΠ°ΠΉΠ½Π΅Π³ΠΎ Π‘Π΅Π²Π΅ΡΠ° ΠΈ ΠΡΠΊΡΠΈΠΊΠΈ
In the Republic of Sakha (Yakutia) there are many winter roads for transportation of food and essential goods. As a rule, vehicles are running on a diesel fuel on such roads. Despite the difficulties in operating diesel vehicles under extremely low temperatures, diesel vehicles are much more powerful and economical than gasoline ones. Problems with start and operation of a diesel engine are associated with low-temperature properties of diesel fuel. The process involved in refining oil to create a winter class diesel fuel is expensive and complex because paraffinic hydrocarbons must be removed.Therefore, today it is important to produce winter classes of diesel fuel by compounding a pour point depressant and a summer class of fuel. When using additives, problems arise with the choice of their concentration. Those limits that the manufacturer recommends in real life show a negative result.There is no wide range of those additives in Yakutia so the authors chose for experiments Dewaxol additives that diminish sedimentation during fuel transportation. So, during the study of the impact of Dewaxol additive, that contained amides and imides of mono- and dicarboxylic acids on the diesel fuel, it was considered how, at various concentrations of the additive and the heating temperature of fuel, the cloud point decreases, and sedimentation stability improves. The least squares method has allowed describing optimal concentration of pour point depressant. The study resulted in the conclusion that the fuel with a high content of depressant-dispersant additive has the best sedimentation stability.Π Π Π΅ΡΠΏΡΠ±Π»ΠΈΠΊΠ΅ Π‘Π°Ρ
Π° (Π―ΠΊΡΡΠΈΡ) ΡΡΠ½ΠΊΡΠΈΠΎΠ½ΠΈΡΡΠ΅Ρ ΠΌΠ½ΠΎΠΆΠ΅ΡΡΠ²ΠΎ Π°Π²ΡΠΎΠ·ΠΈΠΌΠ½ΠΈΠΊΠΎΠ² Π΄Π»Ρ ΠΏΠ΅ΡΠ΅Π²ΠΎΠ·ΠΊΠΈ ΠΏΡΠΎΠ΄ΠΎΠ²ΠΎΠ»ΡΡΡΠ²ΠΈΡ ΠΈ ΡΠΎΠ²Π°ΡΠΎΠ² ΠΏΠ΅ΡΠ²ΠΎΠΉ Π½Π΅ΠΎΠ±Ρ
ΠΎΠ΄ΠΈΠΌΠΎΡΡΠΈ. ΠΠ°ΠΊ ΠΏΡΠ°Π²ΠΈΠ»ΠΎ, ΠΏΠΎ ΡΠ°ΠΊΠΈΠΌ Π΄ΠΎΡΠΎΠ³Π°ΠΌ Π΅Π·Π΄ΡΡ Π°Π²ΡΠΎΠΌΠΎΠ±ΠΈΠ»ΠΈ, ΡΠ°Π±ΠΎΡΠ°ΡΡΠΈΠ΅ Π½Π° Π΄ΠΈΠ·Π΅Π»ΡΠ½ΠΎΠΌ Π΄Π²ΠΈΠ³Π°ΡΠ΅Π»Π΅. ΠΠ΅ΡΠΌΠΎΡΡΡ Π½Π° ΡΡΡΠ΄Π½ΠΎΡΡΠΈ Π² ΡΠΊΡΠΏΠ»ΡΠ°ΡΠ°ΡΠΈΠΈ Π΄ΠΈΠ·Π΅Π»ΡΠ½ΠΎΠΉ ΡΠ΅Ρ
Π½ΠΈΠΊΠΈ ΠΏΡΠΈ ΡΠΊΡΡΡΠ΅ΠΌΠ°Π»ΡΠ½ΠΎ Π½ΠΈΠ·ΠΊΠΈΡ
ΡΠ΅ΠΌΠΏΠ΅ΡΠ°ΡΡΡΠ°Ρ
, Π΄ΠΈΠ·Π΅Π»ΡΠ½Π°Ρ ΡΠ΅Ρ
Π½ΠΈΠΊΠ° Π½Π°ΠΌΠ½ΠΎΠ³ΠΎ ΠΌΠΎΡΠ½Π΅Π΅ ΠΈ ΡΠΊΠΎΠ½ΠΎΠΌΠΈΡΠ½Π΅Π΅ Π±Π΅Π½Π·ΠΈΠ½ΠΎΠ²ΠΎΠΉ. ΠΡΠΎΠ±Π»Π΅ΠΌΡ Ρ Π·Π°ΠΏΡΡΠΊΠΎΠΌ ΠΈ ΡΠ°Π±ΠΎΡΠΎΠΉ Π΄ΠΈΠ·Π΅Π»ΡΠ½ΠΎΠ³ΠΎ Π΄Π²ΠΈΠ³Π°ΡΠ΅Π»Ρ ΡΠ²ΡΠ·Π°Π½Ρ Ρ Π½ΠΈΠ·ΠΊΠΎΡΠ΅ΠΌΠΏΠ΅ΡΠ°ΡΡΡΠ½ΡΠΌΠΈ ΡΠ²ΠΎΠΉΡΡΠ²Π°ΠΌΠΈ Π΄ΠΈΠ·Π΅Π»ΡΠ½ΠΎΠ³ΠΎ ΡΠΎΠΏΠ»ΠΈΠ²Π°. ΠΡΠΎΡΠ΅ΡΡ ΠΏΠ΅ΡΠ΅ΡΠ°Π±ΠΎΡΠΊΠΈ Π½Π΅ΡΡΠΈ Π΄Π»Ρ ΡΠΎΠ·Π΄Π°Π½ΠΈΡ Π·ΠΈΠΌΠ½Π΅Π³ΠΎ ΡΠΎΡΡΠ° Π΄ΠΈΠ·Π΅Π»ΡΠ½ΠΎΠ³ΠΎ ΡΠΎΠΏΠ»ΠΈΠ²Π° ΡΠΎΠΏΡΠΎΠ²ΠΎΠΆΠ΄Π°Π΅ΡΡΡ Π±ΠΎΠ»ΡΡΠΈΠΌΠΈ Π·Π°ΡΡΠ°ΡΠ°ΠΌΠΈ ΠΈ ΡΠ»ΠΎΠΆΠ½ΠΎΠΉ ΡΠ΅Ρ
Π½ΠΎΠ»ΠΎΠ³ΠΈΠ΅ΠΉ, ΠΏΠΎΡΠΎΠΌΡ ΡΡΠΎ Π½Π΅ΠΎΠ±Ρ
ΠΎΠ΄ΠΈΠΌΠΎ ΡΠ΄Π°Π»ΠΈΡΡ ΠΏΠ°ΡΠ°ΡΠΈΠ½ΠΎΠ²ΡΠ΅ ΡΠ³Π»Π΅Π²ΠΎΠ΄ΠΎΡΠΎΠ΄Ρ.ΠΠΎΡΡΠΎΠΌΡ ΡΠ΅Π³ΠΎΠ΄Π½Ρ Π°ΠΊΡΡΠ°Π»ΡΠ½ΠΎ ΠΏΡΠΎΠΈΠ·Π²ΠΎΠ΄ΡΡΠ²ΠΎ Π·ΠΈΠΌΠ½ΠΈΡ
ΡΠΎΡΡΠΎΠ² Π΄ΠΈΠ·Π΅Π»ΡΠ½ΠΎΠ³ΠΎ ΡΠΎΠΏΠ»ΠΈΠ²Π° ΠΏΡΡΡΠΌ ΠΊΠΎΠΌΠΏΠ°ΡΠ½Π΄ΠΈΡΠΎΠ²Π°Π½ΠΈΡ Π΄Π΅ΠΏΡΠ΅ΡΡΠΎΡΠ½ΠΎΠΉ ΠΏΡΠΈΡΠ°Π΄ΠΊΠΈ ΠΈ Π»Π΅ΡΠ½Π΅Π³ΠΎ ΡΠΎΡΡΠ° ΡΠΎΠΏΠ»ΠΈΠ²Π°. ΠΡΠΈ ΠΈΡΠΏΠΎΠ»ΡΠ·ΠΎΠ²Π°Π½ΠΈΠΈ ΠΏΡΠΈΡΠ°Π΄ΠΎΠΊ Π²ΠΎΠ·Π½ΠΈΠΊΠ°ΡΡ ΠΏΡΠΎΠ±Π»Π΅ΠΌΡ Ρ Π²ΡΠ±ΠΎΡΠΎΠΌ ΠΈΡ
ΠΊΠΎΠ½ΡΠ΅Π½ΡΡΠ°ΡΠΈΠΈ. Π’Π΅ ΠΏΡΠ΅Π΄Π΅Π»Ρ, ΠΊΠΎΡΠΎΡΡΠ΅ ΡΠ΅ΠΊΠΎΠΌΠ΅Π½Π΄ΡΠ΅Ρ ΠΏΡΠΎΠΈΠ·Π²ΠΎΠ΄ΠΈΡΠ΅Π»Ρ, Π² ΡΠ΅Π°Π»ΡΠ½ΠΎΠΉ ΠΆΠΈΠ·Π½ΠΈ ΠΏΠΎΠΊΠ°Π·ΡΠ²Π°ΡΡ ΠΎΡΡΠΈΡΠ°ΡΠ΅Π»ΡΠ½ΡΠΉ ΡΠ΅Π·ΡΠ»ΡΡΠ°Ρ.Π Π―ΠΊΡΡΠΈΠΈ ΠΎΡΡΡΡΡΡΠ²ΡΠ΅Ρ ΡΠΈΡΠΎΠΊΠΈΠΉ ΡΠΏΠ΅ΠΊΡΡ ΡΠ°ΠΊΠΈΡ
ΠΏΡΠΈΡΠ°Π΄ΠΎΠΊ, ΠΏΠΎΡΡΠΎΠΌΡ Π°Π²ΡΠΎΡΡ ΠΎΡΡΠ°Π½ΠΎΠ²ΠΈΠ»ΠΈ ΡΠ²ΠΎΠΉ Π²ΡΠ±ΠΎΡ Π΄Π»Ρ ΠΏΡΠΎΠ²Π΅Π΄Π΅Π½ΠΈΡ ΡΠΊΡΠΏΠ΅ΡΠΈΠΌΠ΅Π½ΡΠΎΠ² ΠΏΡΠΈΡΠ°Π΄ΠΊΠ°Ρ
Dewaxol, ΠΊΠΎΡΠΎΡΡΠ΅ ΡΠΌΠ΅Π½ΡΡΠ°ΡΡ ΠΎΡΠ»ΠΎΠΆΠ΅Π½ΠΈΡ ΠΏΡΠΈ ΠΏΠ΅ΡΠ΅Π²ΠΎΠ·ΠΊΠ΅ ΡΠΎΠΏΠ»ΠΈΠ²Π°. Π Ρ
ΠΎΠ΄Π΅ ΠΈΠ·ΡΡΠ΅Π½ΠΈΡ Π²ΠΎΠ·Π΄Π΅ΠΉΡΡΠ²ΠΈΡ ΠΏΡΠΈΡΠ°Π΄ΠΊΠΈ Dewaxol, Π² ΡΠΎΡΡΠ°Π²Π΅ ΠΊΠΎΡΠΎΡΠΎΠΉ Π±ΡΠ»ΠΈ Π°ΠΌΠΈΠ΄Ρ ΠΈ ΠΈΠΌΠΈΠ΄Ρ ΠΌΠΎΠ½ΠΎ- ΠΈ Π΄ΠΈΠΊΠ°ΡΠ±ΠΎΠ½ΠΎΠ²ΡΡ
ΠΊΠΈΡΠ»ΠΎΡ, Π½Π° Π΄ΠΈΠ·Π΅Π»ΡΠ½ΠΎΠ΅ ΡΠΎΠΏΠ»ΠΈΠ²ΠΎ Π±ΡΠ»ΠΎ ΡΠ°ΡΡΠΌΠΎΡΡΠ΅Π½ΠΎ, ΠΊΠ°ΠΊ ΠΏΡΠΈ ΡΠ°Π·Π»ΠΈΡΠ½ΡΡ
ΠΊΠΎΠ½ΡΠ΅Π½ΡΡΠ°ΡΠΈΡΡ
ΠΏΡΠΈΡΠ°Π΄ΠΊΠΈ ΠΈ ΡΠ΅ΠΌΠΏΠ΅ΡΠ°ΡΡΡΠ΅ Π½Π°Π³ΡΠ΅Π²Π° ΡΠΎΠΏΠ»ΠΈΠ²Π° ΡΠ½ΠΈΠΆΠ°Π΅ΡΡΡ ΡΠ΅ΠΌΠΏΠ΅ΡΠ°ΡΡΡΠ° ΠΏΠΎΠΌΡΡΠ½Π΅Π½ΠΈΡ ΠΈ ΡΠ»ΡΡΡΠ°Π΅ΡΡΡ ΡΠ΅Π΄ΠΈΠΌΠ΅Π½ΡΠ°ΡΠΈΠΎΠ½Π½Π°Ρ ΡΡΡΠΎΠΉΡΠΈΠ²ΠΎΡΡΡ. ΠΠ΅ΡΠΎΠ΄ Π½Π°ΠΈΠΌΠ΅Π½ΡΡΠΈΡ
ΠΊΠ²Π°Π΄ΡΠ°ΡΠΎΠ² ΠΏΠΎΠ·Π²ΠΎΠ»ΠΈΠ» ΠΎΠΏΠΈΡΠ°ΡΡ ΠΎΠΏΡΠΈΠΌΠ°Π»ΡΠ½ΡΡ ΠΊΠΎΠ½ΡΠ΅Π½ΡΡΠ°ΡΠΈΡ Π΄Π΅ΠΏΡΠ΅ΡΡΠΎΡΠ½ΠΎΠΉ ΠΏΡΠΈΡΠ°Π΄ΠΊΠΈ. Π ΡΠ΅Π·ΡΠ»ΡΡΠ°ΡΠ΅ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΡ Π²ΡΡΡΠ½ΠΈΠ»ΠΎΡΡ, ΡΡΠΎ Π½Π°ΠΈΠ»ΡΡΡΠ΅ΠΉ ΡΠ΅Π΄ΠΈΠΌΠ΅Π½ΡΠ°ΡΠΈΠΎΠ½Π½ΠΎΠΉ ΡΡΡΠΎΠΉΡΠΈΠ²ΠΎΡΡΡΡ ΠΎΠ±Π»Π°Π΄Π°Π΅Ρ ΡΠΎΠΏΠ»ΠΈΠ²ΠΎ Ρ Π²ΡΡΠΎΠΊΠΈΠΌ ΡΠΎΠ΄Π΅ΡΠΆΠ°Π½ΠΈΠ΅ΠΌ Π΄Π΅ΠΏΡΠ΅ΡΡΠΎΡΠ½ΠΎ-Π΄ΠΈΡΠΏΠ΅ΡΠ³ΠΈΡΡΡΡΠ΅ΠΉ ΠΏΡΠΈΡΠ°Π΄ΠΊΠΈ
Fungal literature records database of the Northern West Siberia (Russia)
Background Mycological research in the Northern part of West Siberia has now become sufficient for review and digitisation as over 460 scientific works have been completed mainly since the beginning of the 20th century. The history of research in the region started from isolated studies at the beginning of the 20th century, but regular and systematic research started from the 1970s. Over the following decades, several dozens of researchers have worked in the area, but the reported occurrences were scattered amongst a broad variety of publications, mainly hardly available. The great need in digitisation and accumulation of fungal records reported in published literature in a standardised regional database has now become evident. The Β«Fungal records database of the Northern West SiberiaΒ» (FuNWS) was initiated in 2016 according to contemporary biodiversity data standards (Darwin Core), to be compatible and accessible by the broad research community. The database has been supplemented ever since by the collective effort of specialists working in the area. According to the database summary report, there are 3358 fungal and fungus-like species revealed in the Northern West Siberia at present. The richest in species number classes are Agaricomycetes (60%) and Lecanoromycetes (33%) with a total of 25 classes represented. The FuNWS database was uploaded to Global Biodiversity Information Facility (GBIF) (Ygra State University Biological Collection publisher) on 11 November 2017 (earlier titled Β«Fungal Records Database of Yugra, FReDYΒ») to provide open access to the data and its reusability (Filippova et al. 2020). New information This publication summarises the results of the digitisation of literature-based occurrence records of fungi and fungus-like organisms initiated in the Northern part of West Siberia for the first time in the history of mycological research. The bibliography of regional mycological publications was created to include about 460 published works (Suppl. material 2). In total, about 140 literature sources were digitised and about 22000 occurrence records were integrated into the FuNWS database (Filippova et al. 2020). Β© Filippova N et al.20-04-00349Russian Foundation for Basic Research,Β ΓΒ ΓΒ€Γۈ : 18-05-00398Russian Foundation for Basic Research,Β ΓΒ ΓΒ€Γۈ : 13-01-20/39,Β 18-44-860017The research was funded by the Russian Fund for Basic Research and Government of the Khanty-Mansiysk Autonomous region according to the research project 18-44-860017 and grant 13-01-20/39 of the Yugra State University. Anton G. Shiryaev was partially funded by the Russian Foundation for Basic Research No 18-05-00398 Π. Elena A. Zvyagina was supported by the KhMAO β Ugra government assignment for Surgut State University β20-04-00349. Π. S. Arefyev was supported by the Fundemental research programme of the Tyumen Scientific Center SB RAS VI.52.1. project number AAAA-A17-117050400146-1. The authors are grateful to Ilya Filippov for preparation of a graph
Hydrometeorological dataset of West Siberian boreal peatland: a 10-year record from the Mukhrino field station
Northern peatlands represent one of the largest carbon pools in the
biosphere, but the carbon they store is increasingly vulnerable to
perturbations from climate and land-use change. Meteorological observations
taken directly at peatland areas in Siberia are unique and rare, while
peatlands are characterized by a specific local climate. This paper presents
a hydrological and meteorological dataset collected at the Mukhrino
peatland, Khanty-Mansi Autonomous Okrug β Yugra, Russia, over the period of
8Β MayΒ 2010 to 31Β DecemberΒ 2019. Hydrometeorological data were collected from
stations located at a small pineβshrubβSphagnum ridge and ScheuchzeriaβSphagnum hollow at ridgeβhollow
complexes of ombrotrophic peatland. The monitored meteorological variables
include air temperature, air humidity, atmospheric pressure, wind speed and
direction, incoming and reflected photosynthetically active radiation, net
radiation, soil heat flux, precipitation (rain), and snow depth. A
gap-filling procedure based on the Gaussian process regression model with an
exponential kernel was developed to obtain continuous time series. For the
record from 2010 to 2019, the average mean annual air temperature at the
site was β1.0ββC, with the mean monthly temperature of the
warmest month (July) recorded as 17.4ββC and for the coldest
month (January) β21.5ββC. The average net radiation was about
35.0βWβmβ2, and the soil heat flux was 2.4 and 1.2βWβmβ2 for the
hollow and the ridge sites, respectively.
The presented data are freely available through Zenodo
(https://doi.org/10.5281/zenodo.4323024, Dyukarev et al.,
2020), last access: 15Β DecemberΒ 2020) and can be used in coordination with
other hydrological and meteorological datasets to examine the
spatiotemporal effects of meteorological conditions on local hydrological
responses across cold regions.</p
Anabar Region of Yakutia in the XX β Early XXI Centuries: Characteristics of the Local Cultural Landscape
The features of the ethnocultural landscape of the Anabar national (Dolgan-Evenk) ulusΒ of the Republic of Sakha (Yakutia) are considered. Attention is paid to the main componentsΒ of cultural landscapes: local communities and traditional economy. In the study area, the retrospective analysis made it possible to identify the dynamics of theΒ number and settlement ofΒ residents, to state the modern functioning of two rural local communities: SaskylakhΒ and Yuryung-khainsky. It is argued that the sustainability and preservation of traditional sectors of theΒ economy are due to the adaptation of the local population to natural landscapes. It is noted thatΒ during the XX β early XXI centuries, the traditional economic activities of the indigenous population, represented by different ethnic groupsΒ that originally inhabited the territory of the ulus,Β remained unchanged and, despite all the socio-economic transformations, remain vital andΒ common for the Anabarians. The article presents the results of the analysis of a sociologicalΒ survey and an associative experiment, which revealed the features of the linguistic landscapeΒ of the area under consideration, depending on different layers of self-awareness: external, withΒ a predominance of Russian-language text in the linguistic appearance of the settlements underΒ study; individual, with a predominance of the Yakut language in intergroup communication; andΒ the subconscious, which revealed the dominance of the Dolgan cultural codes. It has beenΒ established that the cultural landscape of the Anabar ulus is the result ofΒ centuries-old interaction of indigenous ethnic groups inhabiting this area: Dolgans, Evenks, Yakuts and Russians
Π‘ΠΎΡΡΠΎΡΠ½ΠΈΠ΅ Π±Π΅Π·ΠΎΠΏΠ°ΡΠ½ΠΎΡΡΠΈ Π΄ΠΎΡΠΎΠΆΠ½ΠΎΠ³ΠΎ Π΄Π²ΠΈΠΆΠ΅Π½ΠΈΡ Π² ΠΡΠΊΡΠΈΡΠ΅ΡΠΊΠΎΠΉ Π·ΠΎΠ½Π΅ Π ΠΎΡΡΠΈΠΉΡΠΊΠΎΠΉ Π€Π΅Π΄Π΅ΡΠ°ΡΠΈΠΈ
The article deals with the issue of road safety in the Arctic zone of the Russian Federation.The analysis of road traffic accidents over the past 10 years that occurred in the Arctic zone of the Republic of Sakha (Yakutia) was carried out for the first time ever. The study refers to the total number of road traffic accidents, accidents due to the fault of pedestrians, accidents due to the unsatisfied condition of streets and roads, accidents involving children under 16 years of age, accidents involving drivers with signs of alcohol intoxication and accidents committed by drivers without the right to drive vehicles. Based on the data obtained, a coefficient K was proposed that characterises the state of road safety in the Arctic regions in comparison with traffic safety in general in the Republic of Sakha (Yakutia).The analysis of road traffic accident statistics has shown that many accidents are the fault of drivers without a driverβs license and revealed the districts with respectively the highest and lowest number of accidents as per their types listed above.Despite the huge territory and the small number of inhabitants, and consequently the low population density, the number of accidents in the Arctic zone of the Republic of Sakha (Yakutia) has been increasing every year necessitating efforts to improve road safety.Π ΡΡΠ°ΡΡΠ΅ ΡΠ°ΡΡΠΌΠΎΡΡΠ΅Π½ Π²ΠΎΠΏΡΠΎΡ ΠΏΠΎ Π±Π΅Π·ΠΎΠΏΠ°ΡΠ½ΠΎΡΡΠΈ Π΄ΠΎΡΠΎΠΆΠ½ΠΎΠ³ΠΎ Π΄Π²ΠΈΠΆΠ΅Π½ΠΈΡ Π² ΠΡΠΊΡΠΈΡΠ΅ΡΠΊΠΎΠΉ Π·ΠΎΠ½Π΅ Π ΠΎΡΡΠΈΠΉΡΠΊΠΎΠΉ Π€Π΅Π΄Π΅ΡΠ°ΡΠΈΠΈ.ΠΠΏΠ΅ΡΠ²ΡΠ΅ ΠΏΡΠΎΠ²Π΅Π΄ΡΠ½ Π°Π½Π°Π»ΠΈΠ· Π΄ΠΎΡΠΎΠΆΠ½ΠΎ-ΡΡΠ°Π½ΡΠΏΠΎΡΡΠ½ΡΡ
ΠΏΡΠΎΠΈΡΡΠ΅ΡΡΠ²ΠΈΠΉ, ΠΏΡΠΎΠΈΠ·ΠΎΡΠ΅Π΄ΡΠΈΡ
Π½Π° ΡΠ΅ΡΡΠΈΡΠΎΡΠΈΠΈ ΠΡΠΊΡΠΈΡΠ΅ΡΠΊΠΎΠΉ Π·ΠΎΠ½Ρ Π Π΅ΡΠΏΡΠ±Π»ΠΈΠΊΠΈ Π‘Π°Ρ
Π° (Π―ΠΊΡΡΠΈΡ) Π·Π° ΠΏΠΎΡΠ»Π΅Π΄Π½ΠΈΠ΅ Π΄Π΅ΡΡΡΡ Π»Π΅Ρ. ΠΡΠΎΠ°Π½Π°Π»ΠΈΠ·ΠΈΡΠΎΠ²Π°Π½ΠΎ ΠΎΠ±ΡΠ΅Π΅ ΠΊΠΎΠ»ΠΈΡΠ΅ΡΡΠ²ΠΎ ΠΠ’Π, ΠΠ’Π ΠΏΠΎ Π²ΠΈΠ½Π΅ ΠΏΠ΅ΡΠ΅Ρ
ΠΎΠ΄ΠΎΠ², ΠΠ’Π ΠΈΠ·-Π·Π° Π½Π΅ΡΠ΄ΠΎΠ²Π»Π΅ΡΠ²ΠΎΡΠΈΡΠ΅Π»ΡΠ½ΠΎΠ³ΠΎ ΡΠΎΡΡΠΎΡΠ½ΠΈΡ ΡΠ»ΠΈΡ ΠΈ Π΄ΠΎΡΠΎΠ³, ΠΠ’Π Ρ ΡΡΠ°ΡΡΠΈΠ΅ΠΌ Π΄Π΅ΡΠ΅ΠΉ Π΄ΠΎ 16 Π»Π΅Ρ, ΠΠ’Π Ρ ΡΡΠ°ΡΡΠΈΠ΅ΠΌ Π²ΠΎΠ΄ΠΈΡΠ΅Π»Π΅ΠΉ Ρ ΠΏΡΠΈΠ·Π½Π°ΠΊΠ°ΠΌΠΈ ΠΎΠΏΡΡΠ½Π΅Π½ΠΈΡ ΠΈ ΠΠ’Π, Π΄ΠΎΠΏΡΡΠ΅Π½Π½ΡΡ
Π²ΠΎΠ΄ΠΈΡΠ΅Π»ΡΠΌΠΈ Π±Π΅Π· ΠΏΡΠ°Π²Π° Π½Π° ΡΠΏΡΠ°Π²Π»Π΅Π½ΠΈΠ΅ ΡΡΠ°Π½ΡΠΏΠΎΡΡΠ½ΡΠΌΠΈ ΡΡΠ΅Π΄ΡΡΠ²Π°ΠΌΠΈ.ΠΠ° ΠΎΡΠ½ΠΎΠ²Π΅ ΠΏΠΎΠ»ΡΡΠ΅Π½Π½ΡΡ
Π΄Π°Π½Π½ΡΡ
Π±ΡΠ» ΠΏΡΠ΅Π΄Π»ΠΎΠΆΠ΅Π½ ΠΊΠΎΡΡΡΠΈΡΠΈΠ΅Π½Ρ Β«ΠΒ», ΠΊΠΎΡΠΎΡΡΠΉ Ρ
Π°ΡΠ°ΠΊΡΠ΅ΡΠΈΠ·ΡΠ΅Ρ ΡΠΎΡΡΠΎΡΠ½ΠΈΠ΅ Π±Π΅Π·ΠΎΠΏΠ°ΡΠ½ΠΎΡΡΠΈ Π΄ΠΎΡΠΎΠΆΠ½ΠΎΠ³ΠΎ Π΄Π²ΠΈΠΆΠ΅Π½ΠΈΡ Π² ΠΡΠΊΡΠΈΡΠ΅ΡΠΊΠΈΡ
ΡΠ°ΠΉΠΎΠ½Π°Ρ
ΠΏΠΎ ΡΡΠ°Π²Π½Π΅Π½ΠΈΡ Ρ Π±Π΅Π·ΠΎΠΏΠ°ΡΠ½ΠΎΡΡΡΡ Π΄Π²ΠΈΠΆΠ΅Π½ΠΈΡ Π² ΡΠ΅Π»ΠΎΠΌ ΠΏΠΎ Π Π΅ΡΠΏΡΠ±Π»ΠΈΠΊΠ΅ Π‘Π°Ρ
Π° (Π―ΠΊΡΡΠΈΡ).ΠΡΠΎΠ²Π΅Π΄ΡΠ½Π½ΡΠΉ Π°Π½Π°Π»ΠΈΠ· ΡΡΠ°ΡΠΈΡΡΠΈΠΊΠΈ ΠΠ’Π ΠΏΠΎΠΊΠ°Π·Π°Π», ΡΡΠΎ Π±ΠΎΠ»ΡΡΠΎΠ΅ ΠΊΠΎΠ»ΠΈΡΠ΅ΡΡΠ²ΠΎ ΠΠ’Π ΠΏΡΠΎΠΈΡΡ
ΠΎΠ΄ΠΈΡ ΠΏΠΎ Π²ΠΈΠ½Π΅ Π²ΠΎΠ΄ΠΈΡΠ΅Π»Π΅ΠΉ Π±Π΅Π· ΠΏΡΠ°Π² Π½Π° ΡΠΏΡΠ°Π²Π»Π΅Π½ΠΈΠ΅ ΡΡΠ°Π½ΡΠΏΠΎΡΡΠ½ΡΠΌΠΈ ΡΡΠ΅Π΄ΡΡΠ²Π°ΠΌΠΈ. Π’Π°ΠΊΠΆΠ΅ Π±ΡΠ»ΠΈ Π²ΡΡΠ²Π»Π΅Π½Ρ ΡΠ°ΠΉΠΎΠ½Ρ Ρ Π½Π°ΠΈΠ±ΠΎΠ»Π΅Π΅ Π²ΡΡΠΎΠΊΠΈΠΌ ΠΈ Π½ΠΈΠ·ΠΊΠΈΠΌ ΠΊΠΎΠ»ΠΈΡΠ΅ΡΡΠ²ΠΎΠΌ ΠΏΡΠΎΠΈΠ·ΠΎΡΠ΅Π΄ΡΠΈΡ
ΠΠ’Π ΠΏΠΎ ΠΏΠ΅ΡΠ΅ΡΠΈΡΠ»Π΅Π½Π½ΡΠΌ Π²ΡΡΠ΅ Π²ΠΈΠ΄Π°ΠΌ. ΠΠ΅ΡΠΌΠΎΡΡΡ Π½Π° ΠΎΠ³ΡΠΎΠΌΠ½ΡΡ ΡΠ΅ΡΡΠΈΡΠΎΡΠΈΡ ΠΈ Π½Π΅Π±ΠΎΠ»ΡΡΠΎΠ΅ ΡΠΈΡΠ»ΠΎ ΠΆΠΈΡΠ΅Π»Π΅ΠΉ, Π°, ΡΠΎΠΎΡΠ²Π΅ΡΡΡΠ²Π΅Π½Π½ΠΎ, ΠΈ Π½ΠΈΠ·ΠΊΡΡ ΠΏΠ»ΠΎΡΠ½ΠΎΡΡΡ Π½Π°ΡΠ΅Π»Π΅Π½ΠΈΡ, ΠΊΠΎΠ»ΠΈΡΠ΅ΡΡΠ²ΠΎ ΠΠ’Π Π² ΠΡΠΊΡΠΈΡΠ΅ΡΠΊΠΎΠΉ Π·ΠΎΠ½Π΅ Π Π΅ΡΠΏΡΠ±Π»ΠΈΠΊΠΈ Π‘Π°Ρ
Π° (Π―ΠΊΡΡΠΈΡ) ΡΠ²Π΅Π»ΠΈΡΠΈΠ²Π°Π΅ΡΡΡ Ρ ΠΊΠ°ΠΆΠ΄ΡΠΌ Π³ΠΎΠ΄ΠΎΠΌ, ΡΡΠΎ Π΄ΠΈΠΊΡΡΠ΅Ρ ΡΠ΅Π»Π΅ΡΠΎΠΎΠ±ΡΠ°Π·Π½ΠΎΡΡΡ ΠΏΡΠΎΠ²Π΅Π΄Π΅Π½ΠΈΡ ΠΌΠ΅ΡΠΎΠΏΡΠΈΡΡΠΈΠΉ ΠΏΠΎ ΠΏΠΎΠ²ΡΡΠ΅Π½ΠΈΡ Π±Π΅Π·ΠΎΠΏΠ°ΡΠ½ΠΎΡΡΠΈ Π΄ΠΎΡΠΎΠΆΠ½ΠΎΠ³ΠΎ Π΄Π²ΠΈΠΆΠ΅Π½ΠΈΡ
Optical Identification of Four Hard X-ray Sources from the Swift All-Sky Survey
We present the results of our optical identifications of four hard X-ray
sources from the Swift all-sky survey. We obtained optical spectra for each of
the program objects with the 6-m BTA telescope (Special Astrophysical
Observatory, Russian Academy of Sciences, Nizhnii Arkhyz), which allowed their
nature to be established. Two sources (SWIFT J2237.2+6324} and SWIFT
J2341.0+7645) are shown to belong to the class of cataclysmic variables
(suspected polars or intermediate polars). The measured emission line width
turns out to be fairly large (FWHM ~ 15-25 A), suggesting the presence of
extended, rapidly rotating (v~400-600 km/s) accretion disks in the systems.
Apart from line broadening, we have detected a change in the positions of the
line centroids for SWIFT J2341.0+7645, which is most likely attributable to the
orbital motion of the white dwarf in the binary system. The other two program
objects (SWIFT J0003.3+2737 and SWIFT J0113.8+2515) are extragalactic in
origin: the first is a Seyfert 2 galaxy and the second is a blazar at redshift
z=1.594. Apart from the optical spectra, we provide the X-ray spectra for all
sources in the 0.6-10 keV energy band obtained from XRT/Swift data.Comment: 9 pages, 6 figures, will be published in Astronomy Letters, 38, No.5,
pp.281-289 (2012
DIAGNOSTIC MARKERS OF ALLERGIC BRONCHOPULMONARY ASPERGILLOSIS IN PATIENTS WITH BRONCHIAL ASTHMA
Studies of probable significance of different immunological mediators for the development of chronic allergic inflammation in patients with allergic bronchopulmonary aspergillosis (ABPA) are necessary in order to specify potential targets for therapeutic intervention and timely diagnosis of the disease. The purpose of present study was to determine the features of immune response regulation, and to identify diagnostic markers associated with development of ABPA in patients with bronchial asthma, and to evaluate clinical and immunological efficacy of specific antimycotic therapy.The study involved 13 patients with ABPA, 14 patients with bronchial asthma with fungal sensitization (BAFS), 17 patients with bronchial asthma (BA) and 12 apparently healthy individuals. Levels of thymic stromal lymphopoietin (TSLP), thymus and activation-regulated chemokine (TARC), IL-8, as well as levels of total IgE and specific IgE to Aspergillus fumigatus (A. fumigatus) were measured in blood serum by enzyme immunoassay; blood eosinophil counts were also made. Monitoring of these immunological markers in the course of antimycotic therapy was carried out.Significantly higher numbers of eosinophils, increased levels of total IgE and sIgE for A. fumigatus, as well as TARC and IL-8 in serum were revealed in patients with ABPA when compared to the patients with BA. No significant differences in TSLP content were found between the examined groups of patients. A positive correlation between the levels of sIgE to A. fumigatus and contents of TARC and IL-8, numbers of eosinophils, and total IgE levels confirms the important diagnostic value of proinflammatory cytokines in ABPA patients. In the course of itraconazole medication, a positive clinical and immunological dynamics in ABPA patients was revealed. After 12 weeks of therapy, a significant increase in AST, FEV1 and Tiffno respiratory indexes, along with decreased number of eosinophils, total IgE levels, and a trend towards a decrease in TARC and IL-8 levels were documented. This dynamics confirms clinical efficiency of antifungal drugs when treating chronic allergic inflammation in ABPA patients.Implementation of modern immunological biomarkers, alongside with traditional indicators, will allow to differentially evaluate a probability for ABLA development in patients with bronchial asthma, to present additional evidence for discerning early stages of the disease, and to conclude about the efficiency of the therapy applied
Fast optical variability of SS 433
We study the optical variability of the peculiar Galactic source SS 433 using
the observations made with the Russian Turkish 1.5-m telescope (RTT150). A
simple technique which allows to obtain high-quality photometric measurements
with 0.3-1 s time resolution using ordinary CCD is described in detail. Using
the test observations of nonvariable stars, we show that the atmospheric
turbulence introduces no significant distortions into the measured light
curves. Therefore, the data obtained in this way are well suited for studying
the aperiodic variability of various objects.
The large amount of SS 433 optical light curve measurements obtained in this
way allowed us to obtain the power spectra of its flux variability with a
record sensitivity up to frequencies of ~0.5 Hz and to detect its break at
frequency =~2.4e-3 Hz. We suggest that this break in the power spectrum results
from the smoothing of the optical flux variability due to a finite size of the
emitting region. Based on our measurement of the break frequency in the power
spectrum, we estimated the size of the accretion-disk photosphere as 2e12 cm.
We show that the amplitude of the variability in SS 433 decreases sharply
during accretion-disk eclipses, but it does not disappear completely. This
suggests that the size of the variable optical emission source is comparable to
that of the normal star whose size is therefore R_O \approx 2e12 cm \approx 30
R_sun. The decrease in flux variability amplitude during eclipses suggests the
presence of a nonvariable optical emission component with a magnitude
m_R=~13.2.Comment: 12 pages, 11 figures. Accepted for publication in Astronomy Letters.
The original version in Russian is available at
http://hea.iki.rssi.ru/rtt150/ru/ss433_pazh10/pss433_fast.pd
- β¦