Diurnal variations in helium emission

Graphic method for reducing spectrophotoelectric data of twilight helium emissio

An examination of the space-time properties of hydroxyl emission

Spectrometric analysis on space-time properties of hydroxyl emission in various regions of sk

Reverberation measurement of the inner radius of the dust torus in NGC 4151 during 2008-2013

We investigate the correlation between infrared (JHKL) and optical (B) fluxes of the variable nucleus of the Seyfert galaxy NGC 4151 using partially published data for the last 6 years (2008-2013.). Here we are using the same data as in Oknyansky et al. (2014), but include also optical (B) data from Guo et al. We find that the lag of flux in all the infrared bands is the same, 40 +- 6 days, to within the measurement accuracy. Variability in the J and K bands is not quite simultaneous, perhaps due to the differing contributions of the accretion disk in these bands. The lag found for the K band compared with the B band is not significantly different from earlier values obtained for the period 2000-2007. However, finding approximately the same lags in all IR bands for 2008-2013 differs from previous results at earlier epochs when the lag increased with increasing wavelength. Examples of almost the same lag in different IR bands are known for some other active nuclei. In the case of NGC 4151 it appears that the relative lags between the IR bands may be different in different years. The available data, unfortunately, do not allow us to investigate a possible change in the lags during the test interval. We discuss our results in the framework of the standard model where the variable infrared radiation is mainly due to thermal re-emission from the part of the dusty torus closest to the central source. There is also a contribution of some IR emission from the accretion disk, and this contribution increases with decreasing wavelength. Some cosmological applications of obtained results are discussed.Comment: 3 pages, 2 figures, 14-th Odessa International Astronomical Gamow Conference-School Astronomy and beyond: Astrophysics, Cosmology and Gravitation, Cosmomicrophysics, Radio-astronomy and Astrobiolog

Diffraction-limited near-IR imaging at Keck reveals asymmetric, time-variable nebula around carbon star CIT 6

We present multi-epoch, diffraction-limited images of the nebula around the carbon star CIT 6 at 2.2 microns and 3.1 microns from aperture masking on the Keck-I telescope. The near-IR nebula is resolved into two main components, an elongated, bright feature showing time-variable asymmetry and a fainter component about 60 milliarcseconds away with a cooler color temperature. These images were precisely registered (~35 milliarcseconds) with respect to recent visible images from the Hubble Space Telescope (Trammell et al. 2000), which showed a bipolar structure in scattered light. The dominant near-IR feature is associated with the northern lobe of this scattering nebula, and the multi-wavelength dataset can be understood in terms of a bipolar dust shell around CIT 6. Variability of the near-IR morphology is qualitatively consistent with previously observed changes in red polarization, caused by varying illumination geometry due to non-uniform dust production. The blue emission morphology and polarization properties can not be explained by the above model alone, but require the presence of a wide binary companion in the vicinity of the southern polar lobe. The physical mechanisms responsible for the breaking of spherical symmetry around extreme carbon stars, such as CIT 6 and IRC+10216, remain uncertain.Comment: 18 pages, 5 figures (one in color), to appear in the Astrophysical Journa

Structural regularities of welded seam between Ti-Tib and vanadium with 12X18H10T interlayer by using electron beam welding

Досліджувалися можливості отримання зварного з'єднання сплавуТі-TiB заустенітної сталлю 12Х18Н10Т шляхом формування проміжного шару в зварному з'єднанні. Для цього на поверхні зразка сплаву Ті-TiB формувався легований прошарок, що містить армуючі волокна TiB і основні легуючі елементи стали 12Х18Н10Т. Було визначено, що такий прошарок одержується застосуванням електронно-променевого зварювання з'єднання сплаву Ті-TiB з ванадієм через фольгу зі сталі 12Х18Н10Т. Було виявлено, що мікроструктура сформованого прошарку сплаву на основі титану іванадію з легуючими добавками має характер металевої матриці, армованої мікроволокнами, склад яких відповідає боріду титану, легованого ванадієм. Було виявлено, що для армуючих боридних мікроволокон в мікроструктур і прошарку сплаву на основі титану і ванадію характерною особливістю є їх значне подрібнення в порівнянні з вихідним сплавом Ті-TiB. Крім того, в цьому прошарку в зоні розпаду первинних борідів титану, ініційованого впливом електронного променя, були виявлені фазові утворення за елементним складом близькі Ti2B. В результаті було зроблено припущення, що прошарок сплаву на основі Ti (63-68 at.%) І V (18-25 at.%) із легуючими добавками (Fe, Cr, Ni, B, C), сформований на поверхні сплаву Ті -TiB, перспективний для використання для електронно-променевого зварювання сталі 12Х18Н10Т зі сплавом Ті-TiB.Possibilities of obtaining and using an intermediate layer for joining of Ti-TiB and austenitic steel 12X18H10T (analog of AISI 321; 1.4541; X10CrNiTi18-10) were studied. An alloyed interlayer with TiB reinforcing fibers and the main alloying elements of 12X18H10T steel was formed on the surface of the Ti-TiB sample. Such interlayer was formed during electron beam welding of Ti-TiB with vanadium using foil made of 12X18H10T steel. The microstructure of the interlayer consists of a metal matrix reinforced with microfibers. It’s composition corresponds to vanadium-alloyed titanium boride. In comparison to the initial Ti-TiB alloy, significant grinding of reinforcing boride microfibers in the interlayer microstructure was observed. Besides, the phase formations close to Ti2B in zone of primary titanium borides decomposition in the interlayer, initiated by electron beam were determined. As a result, application of Ti (63–68 at. %) and V (18–25 at. %) based interlayer with alloying additives (Fe, Cr, Ni, B, C) has great potential for utilization in electron-beam welding of 12Х18Н10Т steel with Ti-TiB alloy.Исследовались возможности получения и использования промежуточной прослойки для выполнения сварного соединения сплава Ті-TiB с аустенитной сталью 12Х18Н10Т (аналоги AISI 321, 1.4541, X10CrNiTi18-10). Для этого на поверхности образца сплава Ті-TiB формировалась легированная прослойка, содержащая армирующие волокна TiB и основные легирующие элементы стали 12Х18Н10Т. Было определено, что такая прослойка получается применением электронно-лучевой сварки соединения сплава Ті-TiB с ванадием через фольгу из стали 12Х18Н10Т. Было выявлено, что микроструктура сформированной прослойки сплава на основе титана и ванадия с легирующими добавками имеет характер металлической матрицы, армированной микроволокнами, состав которых соответствует бориду титана, легированногованадием. Былообнаружено, что для армирующих боридных микроволокон в микроструктуре прослойки сплава на основе титана и ванадия характерной особенностью является их значительно еизмельчение в сравнении с исходным сплавом Ті-TiB. Кроме того, в этой прослойке в зоне распада первичных боридо втитана, инициированного влиянием электронного луча, были обнаружены фазовые образования по элементному составу близкие Ti2B. В результате было сделано предположение, что прослойка сплава на основе Ti (63–68 at. %) и V (18–25 at. %) с легирующими добавками (Fe, Cr, Ni, B, C), сформированная на поверхности сплава Ті-TiB, перспективна для использования для электронно-лучевой сварки стали 12Х18Н10Т со сплавом Ті-TiB

Pivotal Advance: Eosinophil infiltration of solid tumors is an early and persistent inflammatory host response

Tumor-associated eosinophilia has been observed in numerous human cancers and several tumor models in animals; however, the details surrounding this eosinophilia remain largely undefined and anecdotal. We used a B16-F10 melanoma cell injection model to demonstrate that eosinophil infiltration of tumors occurred from the earliest palpable stages with significant accumulations only in the necrotic and capsule regions. Furthermore, the presence of diffuse extracellular matrix staining for eosinophil major basic protein was restricted to the necrotic areas of tumors, indicating that eosinophil degranulation was limited to this region. Antibody-mediated depletion of CD4+ T cells and adoptive transfer of eosinophils suggested, respectively, that the accumulation of eosinophils is not associated with T helper cell type 2-dependent immune responses and that recruitment is a dynamic, ongoing process, occurring throughout tumor growth. Ex vivo migration studies have identified what appears to be a novel chemotactic factor(s) released by stressed/dying melanoma cells, suggesting that the accumulation of eosinophils in tumors occurs, in part, through a unique mechanism dependent on a signal(s) released from areas of necrosis. Collectively, these studies demonstrate that the infiltration of tumors by eosinophils is an early and persistent response that is spatial-restricted. It is more important that these data also show that the mechanism(s) that elicit this host response occur, independent of immune surveillance, suggesting that eosinophils are part of an early inflammatory reaction at the site of tumorigenesis. © Society for Leukocyte Biology

The central binary and surrounding nebula of the symbiotic star V1016 Cygni

We present HST/WFPC2 images of the symbiotic star V1016 Cyg which, for the first time, directly explore the inner regions of the nebula to AU scales at optical wavelengths. They also suggest that the [OIII] 4959,5007 emission takes place in a bipolar outflow. We use these images to determine the position of the two stars and hence a projected binary separation of 84 AU (assuming a distance of 2 kpc) and a position angle of 143.5 degrees. Furthermore, we combine our images with VLA radio imaging which enables diagnostic tests to be applied and properties of the circumstellar nebula to be determined. Finally we have obtained archive HST/STIS spectra of V1016 Cyg with which we were able to spatially resolve the source at various positions in the nebula. This enabled discovery of the ultraviolet counterpart to the ~25 arcsec extended emission found by Bang et al. (1992).Comment: Accepted for publication in Ap