16 research outputs found
Radiation induced warping of protostellar accretion disks
We examine the consequences of radiatively driven warping of accretion disks
surrounding pre-main-sequence stars. These disks are stable against warping if
the luminosity arises from a steady accretion flow, but are unstable at late
times when the intrinsic luminosity of the star overwhelms that provided by the
disk. Warps can be excited for stars with luminosities of around 10 solar
luminosities or greater, with larger and more severe warps in the more luminous
systems. A twisted inner disk may lead to high extinction towards stars often
viewed through their disks. After the disk at all radii becomes optically thin,
the warp decays gradually on the local viscous timescale, which is likely to be
long. We suggest that radiation induced warping may account for the origin of
the warped dust disk seen in Beta Pictoris, if the star is only around 10-20
Myr old, and could lead to non-coplanar planetary systems around higher mass
stars.Comment: 12 pages, including 3 figures. ApJ Letters, in pres
ΠΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΠ΅ ΡΠΈΠ·ΠΈΡΠ΅ΡΠΊΠΈΡ ΡΠ²Π»Π΅Π½ΠΈΠΉ Π² Π±Π°ΡΠ±ΠΎΡΠ°ΠΆΠ½ΠΎΠΉ Π·ΠΎΠ½Π΅ ΠΏΠ»Π°Π²ΠΈΠ»ΡΠ½ΠΎΠ³ΠΎ Π°Π³ΡΠ΅Π³Π°ΡΠ° Β«ΠΠΎΠ±Π΅Π΄Π°Β» ΠΌΠ΅ΡΠΎΠ΄ΠΎΠΌ Ρ ΠΎΠ»ΠΎΠ΄Π½ΠΎΠ³ΠΎ ΠΌΠΎΠ΄Π΅Π»ΠΈΡΠΎΠ²Π°Π½ΠΈΡ Π‘ΠΎΠΎΠ±ΡΠ΅Π½ΠΈΠ΅ 3. ΠΠΈΠ΄ΡΠΎΠ³Π°Π·ΠΎΠ΄ΠΈΠ½Π°ΠΌΠΈΠΊΠ° ΠΊΠΎΠΌΠ±ΠΈΠ½ΠΈΡΠΎΠ²Π°Π½Π½ΠΎΠΉ ΠΏΡΠΎΠ΄ΡΠ²ΠΊΠΈ ΠΆΠΈΠ΄ΠΊΠΎΡΡΠΈ Π³Π°Π·ΠΎΠΌ Ρ ΠΏΠΎΠΌΠΎΡΡΡ Π΄ΠΎΠ½Π½ΠΎΠΉ ΠΈ Π±ΠΎΠΊΠΎΠ²ΠΎΠΉ ΡΡΡΠΌ
Hydro-gas regularities of liquid combined blowing by gas were studied using cold modeling method at Archimedes criterion for lateral Arl = 12Γ·120 and bottom blowing Arb = 5Γ·60 simulating Pobeda bubbling unit. The blowing was performed simultaneously by bottom lance vertically fixed in centre of reactor and by the lateral lance which was attached at an angle 5Β° to the horizontal axis. The quantitative estimation of instantaneous and average circulation velocities (Vav) of liquid flow elements in different bath areas, depending on the location of blowing zone and Archimedes criterion, was performed. The liquid motion trajectory was determined. A vortex zone was revealed near the liquid surface and the reactor shell, where instantaneous velocity of the liquid flow elements changes from 69.9 to 181.1 mm/s and Vav = 123.8 mm/s. The circulation flows fade in the bulk of liquid and Vav decreases from 123.8 to 47.0 and 54.1 mm/s. It was shown that, in general, circulation velocity depends on the blowing intensity and appears to be higher for the zone of overlapping of lateral and bottom streams. The dynamic blowing conditions, which ensure the direct contact of lateral and bottom jets leading to their interflow and increased spatter formation, were identified. The characteristics of 3 types of surface oscillations for interface phases βpure liquid- gas-liquid layerβ, as well as the estimation of the lateral and bottom blowing impact on the type of oscillation were provided. It has been noted that the introduction of the bottom blowing (Arb = 5) causes the wave-like motion of liquid (the 2nd type) along with the transverse oscillations of the 1st type, and at higher values of Arb = 25 the angular oscillations of the 3rd type develop. It has been shown that the presence of a lateral jet at the combined blowing decreases angles of bath swinging to 8β12Β° to horizontal axis. For the estimation of oscillation intensity, Ξhl = (hl )max β (hl )min value, which means the difference between maximum (hl )max and minimum (hl )min height of liquid for the full-wave oscillations (Ο), was introduced. The height of liquid (hl ) was plotted as a function of Ο, Arl , Arb, Ξhl was determined on the basis of obtained graph values, which varied upon modeling over the range of 7.7β69.5 mm. The relation between the liquid circulation velocity and the oscillation value (Ξhl ) was established for different bath zones and dynamic conditions of the blowing. The impact of all oscillations types on potential erosive lining wear of Pobeda bubbling unit and the completeness of adoption of charging material nearby the bath surface was investigated.ΠΠ΅ΡΠΎΠ΄ΠΎΠΌ Ρ
ΠΎΠ»ΠΎΠ΄Π½ΠΎΠ³ΠΎ ΠΌΠΎΠ΄Π΅Π»ΠΈΡΠΎΠ²Π°Π½ΠΈΡ Π² ΠΈΠ½ΡΠ΅ΡΠ²Π°Π»Π°Ρ
Π²Π΅Π»ΠΈΡΠΈΠ½ ΠΊΡΠΈΡΠ΅ΡΠΈΡ ΠΡΡ
ΠΈΠΌΠ΅Π΄Π° Π΄Π»Ρ Π±ΠΎΠΊΠΎΠ²ΠΎΠ³ΠΎ (ArΠ± = 12Γ·120) ΠΈ Π΄ΠΎΠ½Π½ΠΎΠ³ΠΎ (ArΠ΄ = 5Γ·60) Π΄ΡΡΡΡ ΠΏΡΠΈΠΌΠ΅Π½ΠΈΡΠ΅Π»ΡΠ½ΠΎ ΠΊ ΡΡΠ»ΠΎΠ²ΠΈΡΠΌ ΡΠ°Π±ΠΎΡΡ Π±Π°ΡΠ±ΠΎΡΠ°ΠΆΠ½ΠΎΠ³ΠΎ ΠΏΠ»Π°Π²ΠΈΠ»ΡΠ½ΠΎΠ³ΠΎ Π°Π³ΡΠ΅Π³Π°ΡΠ° Β«ΠΠΎΠ±Π΅Π΄Π°Β» (ΠΠΠ) ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½Ρ Π³ΠΈΠ΄ΡΠΎΠ³Π°Π·ΠΎΠ΄ΠΈΠ½Π°ΠΌΠΈΡΠ΅ΡΠΊΠΈΠ΅ Π·Π°ΠΊΠΎΠ½ΠΎΠΌΠ΅ΡΠ½ΠΎΡΡΠΈ ΠΊΠΎΠΌΠ±ΠΈΠ½ΠΈΡΠΎΠ²Π°Π½Π½ΠΎΠΉ ΠΏΡΠΎΠ΄ΡΠ²ΠΊΠΈ ΠΆΠΈΠ΄ΠΊΠΎΡΡΠΈ Π³Π°Π·ΠΎΠΌ. ΠΡΠΎΠ΄ΡΠ²ΠΊΡ ΠΎΡΡΡΠ΅ΡΡΠ²Π»ΡΠ»ΠΈ ΠΎΠ΄Π½ΠΎΠ²ΡΠ΅ΠΌΠ΅Π½Π½ΠΎ Π΄ΠΎΠ½Π½ΠΎΠΉ ΡΡΡΠΌΠΎΠΉ, ΡΡΡΠ°Π½ΠΎΠ²Π»Π΅Π½Π½ΠΎΠΉ Π²Π΅ΡΡΠΈΠΊΠ°Π»ΡΠ½ΠΎ ΠΏΠΎ ΡΠ΅Π½ΡΡΡ ΡΠ΅Π°ΠΊΡΠΎΡΠ°, ΠΈ Π±ΠΎΠΊΠΎΠ²ΠΎΠΉ, ΡΠ°ΡΠΏΠΎΠ»ΠΎΠΆΠ΅Π½Π½ΠΎΠΉ ΠΏΠΎΠ΄ ΡΠ³Π»ΠΎΠΌ 5Β° ΠΊ Π³ΠΎΡΠΈΠ·ΠΎΠ½ΡΠ°Π»ΡΠ½ΠΎΠΉ ΠΎΡΠΈ. ΠΡΠΎΠ²Π΅Π΄Π΅Π½Π° ΠΊΠΎΠ»ΠΈΡΠ΅ΡΡΠ²Π΅Π½Π½Π°Ρ ΠΎΡΠ΅Π½ΠΊΠ° ΠΌΠ³Π½ΠΎΠ²Π΅Π½Π½ΠΎΠΉ ΠΈ ΡΡΠ΅Π΄Π½Π΅ΠΉ (VΡΡ) ΡΠΊΠΎΡΠΎΡΡΠ΅ΠΉ ΡΠΈΡΠΊΡΠ»ΡΡΠΈΠΈ ΡΠ»Π΅ΠΌΠ΅Π½ΡΠΎΠ² ΠΏΠΎΡΠΎΠΊΠ° ΠΆΠΈΠ΄ΠΊΠΎΡΡΠΈ Π½Π° ΡΠ°Π·Π½ΡΡ
ΡΡΠ°ΡΡΠΊΠ°Ρ
Π²Π°Π½Π½Ρ Π² Π·Π°Π²ΠΈΡΠΈΠΌΠΎΡΡΠΈ ΠΎΡ ΠΌΠ΅ΡΡΠΎΠ½Π°Ρ
ΠΎΠΆΠ΄Π΅Π½ΠΈΡ Π·ΠΎΠ½Ρ ΠΏΡΠΎΠ΄ΡΠ²ΠΊΠΈ ΠΈ ΠΊΡΠΈΡΠ΅ΡΠΈΠ΅Π² ΠΡΡ
ΠΈΠΌΠ΅Π΄Π°. ΠΠΏΡΠ΅Π΄Π΅Π»Π΅Π½Π° ΡΡΠ°Π΅ΠΊΡΠΎΡΠΈΡ Π΄Π²ΠΈΠΆΠ΅Π½ΠΈΡ ΠΆΠΈΠ΄ΠΊΠΎΡΡΠΈ. ΠΠ±Π»ΠΈΠ·ΠΈ ΠΏΠΎΠ²Π΅ΡΡ
Π½ΠΎΡΡΠΈ ΠΆΠΈΠ΄ΠΊΠΎΡΡΠΈ ΠΈ ΠΊΠΎΡΠΏΡΡΠ° ΡΠ΅Π°ΠΊΡΠΎΡΠ° ΠΎΠ±Π½Π°ΡΡΠΆΠ΅Π½Π° Π²ΠΈΡ
ΡΠ΅Π²Π°Ρ Π·ΠΎΠ½Π°, Π³Π΄Π΅ ΠΌΠ³Π½ΠΎΠ²Π΅Π½Π½Π°Ρ ΡΠΊΠΎΡΠΎΡΡΡ Π΄Π²ΠΈΠΆΠ΅Π½ΠΈΡ ΡΠ»Π΅ΠΌΠ΅Π½ΡΠ° ΠΏΠΎΡΠΎΠΊΠ° ΠΆΠΈΠ΄ΠΊΠΎΡΡΠΈ ΠΈΠ·ΠΌΠ΅Π½ΡΠ΅ΡΡΡ ΠΎΡ 69,9 Π΄ΠΎ 183,1 ΠΌΠΌ/Ρ ΠΈ VΡΡ = 123,8 ΠΌΠΌ/Ρ. Π ΠΎΠ±ΡΠ΅ΠΌΠ΅ ΠΆΠΈΠ΄ΠΊΠΎΡΡΠΈ ΡΠΈΡΠΊΡΠ»ΡΡΠΈΠΎΠ½Π½ΡΠ΅ ΠΏΠΎΡΠΎΠΊΠΈ Π·Π°ΡΡΡ
Π°ΡΡ, ΠΈ VΡΡ ΡΠΌΠ΅Π½ΡΡΠ°Π΅ΡΡΡ ΠΎΡ 123,8 Π΄ΠΎ 47,0 ΠΈ 54,1 ΠΌΠΌ/Ρ. ΠΠΎΠΊΠ°Π·Π°Π½ΠΎ, ΡΡΠΎ Π² ΠΎΠ±ΡΠ΅ΠΌ ΡΠ»ΡΡΠ°Π΅ ΡΠΊΠΎΡΠΎΡΡΡ ΡΠΈΡΠΊΡΠ»ΡΡΠΈΠΈ Π·Π°Π²ΠΈΡΠΈΡ ΠΎΡ ΠΈΠ½ΡΠ΅Π½ΡΠΈΠ²Π½ΠΎΡΡΠΈ ΠΏΡΠΎΠ΄ΡΠ²ΠΊΠΈ Π½Π° ΡΡΡΠΌΠ°Ρ
ΠΈ ΡΡΠ°Π½ΠΎΠ²ΠΈΡΡΡ Π²ΡΡΠ΅ Π΄Π»Ρ ΠΎΠ±Π»Π°ΡΡΠΈ Π½Π°Π»ΠΎΠΆΠ΅Π½ΠΈΡ Π±ΠΎΠΊΠΎΠ²ΠΎΠΉ ΠΈ Π΄ΠΎΠ½Π½ΠΎΠΉ ΡΡΡΡΠΉ. ΠΠΏΡΠ΅Π΄Π΅Π»Π΅Π½Ρ Π΄ΠΈΠ½Π°ΠΌΠΈΡΠ΅ΡΠΊΠΈΠ΅ ΡΡΠ»ΠΎΠ²ΠΈΡ ΠΏΡΠΎΠ΄ΡΠ²ΠΊΠΈ, ΠΎΠ±Π΅ΡΠΏΠ΅ΡΠΈΠ²Π°ΡΡΠΈΠ΅ Π½Π΅ΠΏΠΎΡΡΠ΅Π΄ΡΡΠ²Π΅Π½Π½ΡΠΉ ΠΊΠΎΠ½ΡΠ°ΠΊΡ Π±ΠΎΠΊΠΎΠ²ΠΎΠ³ΠΎ ΠΈ Π΄ΠΎΠ½Π½ΠΎΠ³ΠΎ ΡΠ°ΠΊΠ΅Π»ΠΎΠ², ΠΏΡΠΈΠ²ΠΎΠ΄ΡΡΠΈΠΉ ΠΊ ΡΠ»ΠΈΡΠ½ΠΈΡ ΠΏΠΎΡΠΎΠΊΠΎΠ² ΠΈ ΠΏΠΎΠ²ΡΡΠ΅Π½Π½ΠΎΠΌΡ Π±ΡΡΠ·Π³ΠΎΠΎΠ±ΡΠ°Π·ΠΎΠ²Π°Π½ΠΈΡ. ΠΡΠΈΠ²Π΅Π΄Π΅Π½Π° Ρ
Π°ΡΠ°ΠΊΡΠ΅ΡΠΈΡΡΠΈΠΊΠ° 3 Π²ΠΈΠ΄ΠΎΠ² ΠΊΠΎΠ»Π΅Π±Π°Π½ΠΈΠΉ ΠΏΠΎΠ²Π΅ΡΡ
Π½ΠΎΡΡΠΈ ΡΠ°Π·Π΄Π΅Π»Π° ΡΠ°Π· Β«ΡΠΈΡΡΠ°Ρ ΠΆΠΈΠ΄ΠΊΠΎΡΡΡ β Π³Π°Π·ΠΎΠΆΠΈΠ΄ΠΊΠΎΡΡΠ½ΡΠΉ ΡΠ»ΠΎΠΉΒ» ΠΈ Π΄Π°Π½Π° ΠΎΡΠ΅Π½ΠΊΠ° Π²Π»ΠΈΡΠ½ΠΈΡ Π±ΠΎΠΊΠΎΠ²ΠΎΠ³ΠΎ ΠΈ Π΄ΠΎΠ½Π½ΠΎΠ³ΠΎ Π΄ΡΡΡΡ Π½Π° ΡΠ°Π·Π½ΠΎΠ²ΠΈΠ΄Π½ΠΎΡΡΡ Π²ΠΎΠ·Π½ΠΈΠΊΠ°ΡΡΠΈΡ
ΠΊΠΎΠ»Π΅Π±Π°Π½ΠΈΠΉ. ΠΡΠΌΠ΅ΡΠ΅Π½ΠΎ, ΡΡΠΎ Π²Π²ΠΎΠ΄ Π΄ΠΎΠ½Π½ΠΎΠ³ΠΎ Π΄ΡΡΡΡ (ArΠ΄ = 5) ΠΏΡΠΈΠ²ΠΎΠ΄ΠΈΡ, Π½Π°ΡΡΠ΄Ρ Ρ ΠΏΠΎΠΏΠ΅ΡΠ΅ΡΠ½ΡΠΌΠΈ ΠΊΠΎΠ»Π΅Π±Π°Π½ΠΈΡΠΌΠΈ 1-Π³ΠΎ ΡΠΈΠΏΠ°, ΠΊ ΠΏΠΎΡΠ²Π»Π΅Π½ΠΈΡ Π²ΠΎΠ»Π½ΠΎΠΎΠ±ΡΠ°Π·Π½ΠΎΠ³ΠΎ Π΄Π²ΠΈΠΆΠ΅Π½ΠΈΡ ΠΆΠΈΠ΄ΠΊΠΎΡΡΠΈ (2-ΠΉ ΡΠΈΠΏ), Π° ΠΏΡΠΈ Π±ΠΎΠ»Π΅Π΅ Π²ΡΡΠΎΠΊΠΈΡ
Π·Π½Π°ΡΠ΅Π½ΠΈΡΡ
ArΠ΄ = 25 β ΠΊ ΡΠ³Π»ΠΎΠ²ΡΠΌ ΠΊΠΎΠ»Π΅Π±Π°Π½ΠΈΡΠΌ (3-ΠΉ ΡΠΈΠΏ). ΠΠΎΠΊΠ°Π·Π°Π½ΠΎ, ΡΡΠΎ ΠΏΡΠΈ ΠΊΠΎΠΌΠ±ΠΈΠ½ΠΈΡΠΎΠ²Π°Π½Π½ΠΎΠΉ ΠΏΡΠΎΠ΄ΡΠ²ΠΊΠ΅ Π½Π°Π»ΠΈΡΠΈΠ΅ Π±ΠΎΠΊΠΎΠ²ΠΎΠ³ΠΎ ΡΠ°ΠΊΠ΅Π»Π° ΡΠΌΠ΅Π½ΡΡΠ°Π΅Ρ ΡΠ³Π»Ρ ΡΠ°ΡΠΊΠ°ΡΠΈΠ²Π°Π½ΠΈΡ Π²Π°Π½Π½Ρ ΠΊ Π³ΠΎΡΠΈΠ·ΠΎΠ½ΡΡ Π΄ΠΎ 8β12Β°. ΠΠ»Ρ ΠΎΡΠ΅Π½ΠΊΠΈ ΠΈΠ½ΡΠ΅Π½ΡΠΈΠ²Π½ΠΎΡΡΠΈ ΠΊΠΎΠ»Π΅Π±Π°Π½ΠΈΠΉ Π²Π²Π΅Π΄Π΅Π½Π° Π²Π΅Π»ΠΈΡΠΈΠ½Π° ΞhΠΆ = (hΠΆ)max β (hΠΆ)min, Ρ.Π΅. ΡΠ°Π·Π½ΠΎΡΡΡ ΠΌΠ΅ΠΆΠ΄Ρ ΠΌΠ°ΠΊΡΠΈΠΌΠ°Π»ΡΠ½ΠΎΠΉ (hΠΆ)max ΠΈ ΠΌΠΈΠ½ΠΈΠΌΠ°Π»ΡΠ½ΠΎΠΉ (hΠΆ)min Π²ΡΡΠΎΡΠΎΠΉ ΠΆΠΈΠ΄ΠΊΠΎΡΡΠΈ Π·Π° ΠΏΠΎΠ»Π½ΡΠΉ ΡΠΈΠΊΠ» ΠΊΠΎΠ»Π΅Π±Π°Π½ΠΈΠΉ (Ο). ΠΠΎΡΡΡΠΎΠ΅Π½Ρ Π·Π°Π²ΠΈΡΠΈΠΌΠΎΡΡΠΈ Π²ΡΡΠΎΡΡ ΠΆΠΈΠ΄ΠΊΠΎΡΡΠΈ (hΠΆ) ΠΎΡ Ο, ArΠ± ΠΈ ArΠ΄, Π½Π° ΠΎΡΠ½ΠΎΠ²Π°Π½ΠΈΠΈ ΠΊΠΎΡΠΎΡΡΡ
ΠΎΠΏΡΠ΅Π΄Π΅Π»Π΅Π½Ρ Π²Π΅Π»ΠΈΡΠΈΠ½Ρ ΞhΠΆ, Π²Π°ΡΡΠΈΡΡΠ΅ΠΌΡΠ΅ ΠΏΡΠΈ ΠΌΠΎΠ΄Π΅Π»ΠΈΡΠΎΠ²Π°Π½ΠΈΠΈ Π² ΠΈΠ½ΡΠ΅ΡΠ²Π°Π»Π΅ 7,7β69,5 ΠΌΠΌ. ΠΠ»Ρ ΡΠ°Π·Π»ΠΈΡΠ½ΡΡ
ΠΎΠ±Π»Π°ΡΡΠ΅ΠΉ Π²Π°Π½Π½Ρ ΠΈ Π΄ΠΈΠ½Π°ΠΌΠΈΡΠ΅ΡΠΊΠΈΡ
ΡΡΠ»ΠΎΠ²ΠΈΠΉ ΠΏΡΠΎΠ΄ΡΠ²ΠΊΠΈ ΡΡΡΠ°Π½ΠΎΠ²Π»Π΅Π½Π° Π²Π·Π°ΠΈΠΌΠΎΡΠ²ΡΠ·Ρ ΠΌΠ΅ΠΆΠ΄Ρ ΡΠΊΠΎΡΠΎΡΡΡΡ ΡΠΈΡΠΊΡΠ»ΡΡΠΈΠΈ ΠΆΠΈΠ΄ΠΊΠΎΡΡΠΈ ΠΈ Π²Π΅Π»ΠΈΡΠΈΠ½ΠΎΠΉ ΠΊΠΎΠ»Π΅Π±Π°Π½ΠΈΠΉ (ΞhΠΆ). Π Π°ΡΡΠΌΠΎΡΡΠ΅Π½ΠΎ Π²Π»ΠΈΡΠ½ΠΈΠ΅ Π²ΡΠ΅Ρ
Π²ΠΈΠ΄ΠΎΠ² ΠΊΠΎΠ»Π΅Π±Π°Π½ΠΈΠΉ Π½Π° Π²ΠΎΠ·ΠΌΠΎΠΆΠ½ΡΠΉ ΡΡΠΎΠ·ΠΈΠ²Π½ΡΠΉ ΠΈΠ·Π½ΠΎΡ ΡΡΡΠ΅ΡΠΎΠ²ΠΊΠΈ ΠΠΠ ΠΈ ΠΏΠΎΠ»Π½ΠΎΡΡ ΡΡΠ²ΠΎΠ΅Π½ΠΈΡ ΡΠΈΡ
ΡΠΎΠ²ΡΡ
ΠΌΠ°ΡΠ΅ΡΠΈΠ°Π»ΠΎΠ² Π²Π±Π»ΠΈΠ·ΠΈ ΠΏΠΎΠ²Π΅ΡΡ
Π½ΠΎΡΡΠΈ Π²Π°Π½Π½Ρ
A catalogue of dense cores and young stellar objects in the Lupus complex based on Herschel Gould Belt Survey observations
Context. How the diffuse medium of molecular clouds condenses in dense cores and how many of these cores will evolve in protostars is still a poorly understood step of the star formation process. Much progress is being made in this field, thanks to the extensive imaging of star-forming regions carried out with the Herschel Space Observatory.
Aims. The Herschel Gould Belt Survey key project mapped the bulk of nearby star-forming molecular clouds in five far-infrared bands with the aim of compiling complete census of prestellar cores and young, embedded protostars. From the complete sample of prestellar cores, we aim at defining the core mass function and studying its relationship with the stellar initial mass function. Young stellar objects (YSOs) with a residual circumstellar envelope are also detected.
Methods. In this paper, we present the catalogue of the dense cores and YSOs/protostars extracted from the Herschel maps of the Lupus I, III, and IV molecular clouds. The physical properties of the detected objects were derived by fitting their spectral energy distributions.
Results. A total of 532 dense cores, out of which 103 are presumably prestellar in nature, and 38 YSOs/protostars have been detected in the three clouds. Almost all the prestellar cores are associated with filaments against only about one third of the unbound cores and YSOs/protostars. Prestellar core candidates are found even in filaments that are on average thermally subcritical and over a background column density lower than that measured in other star-forming regions so far. The core mass function of the prestellar cores peaks between 0.2 and 0.3 Mβ, and it is compatible with the log-normal shape found in other regions. Herschel data reveal several, previously undetected, protostars and new candidates of Class 0 and Class II with transitional disks. We estimate the evolutionary status of the YSOs/protostars using two independent indicators: the Ξ± index and the fitting of the spectral energy distribution from near- to far-infrared wavelengths. For 70% of the objects, the evolutionary stages derived with the two methods are in agreement.
Conclusions. Lupus is confirmed to be a very low-mass star-forming region, in terms of both the prestellar condensations and the diffuse medium. Noticeably, in the Lupus clouds we have found star formation activity associated with interstellar medium at low column density, usually quiescent in other (more massive) star-forming regions
ΠΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΠ΅ Π½Π°ΡΡΡΠ΅Π½ΠΈΠΉ ΡΡΠ½ΠΊΡΠΈΠΎΠ½Π°Π»ΡΠ½ΡΡ ΡΠ²ΡΠ·Π΅ΠΉ ΠΌΠ΅ΠΆΠ΄Ρ ΡΠ΅ΡΡΡ ΠΏΠ°ΡΡΠΈΠ²Π½ΠΎΠ³ΠΎ ΡΠ΅ΠΆΠΈΠΌΠ° ΡΠ°Π±ΠΎΡΡ ΠΌΠΎΠ·Π³Π° ΠΈ ΡΡΡΡΠΊΡΡΡΠ°ΠΌΠΈ ΠΌΠΎΠ·ΠΆΠ΅ΡΠΊΠ° Ρ ΠΏΠ°ΡΠΈΠ΅Π½ΡΠΎΠ² Ρ Π»Π΅Π³ΠΊΠΎΠΉ ΡΠ΅ΡΠ΅ΠΏΠ½ΠΎ-ΠΌΠΎΠ·Π³ΠΎΠ²ΠΎΠΉ ΡΡΠ°Π²ΠΌΠΎΠΉ Π² ΠΎΡΡΡΠΎΠΉ ΡΡΠ°Π΄ΠΈΠΈ ΠΏΠΎ Π΄Π°Π½Π½ΡΠΌ ΡΠΠ Π’ ΡΠΎΡΡΠΎΡΠ½ΠΈΡ ΠΏΠΎΠΊΠΎΡ
Mild traumatic brain injury (mTBI) is the most common neurological damage in children that's why it is extremely important to identify and analyze biomarkers that can help in predicting patient's treatment and recovery in period of mTBI. Aim of this study is to verify a hypothesis that functional connectivity disturbances between intact cerebellum and DMN nodes are included in symptomatic manifestation of mTBI.Methods. 28 MR negative patients with mTBI were studied in age from 12 to 17 years (mean age β 14.7 years). The control group consisted of 23 healthy children. All MRI studies wereperformed on a Philips AchievadStream 3.0 T scanner equipped with a 32-channelPhilips dStream head coil. A 4 min rsfMRI gradient-echo echo planar imaging (EPI)sequence was acquired (TR = 3000 ms, echo time (TE) = 30 ms, 80 dynamics withdynamic scan time = 3 s). fMRI data were processed using functional connectivitytoolbox CONN.Results. No statistically significant differences in correlation strengths between control group and group of patients were detected as a result of DMN analysis. Intergroup seed-basedcorrelation ROI analysis revealed statistically significant (p < 0.05) differencein links between DMN regions and vermis (cerebellum): positive link in control group and negative link in groupof patients.Conclusions. The revealed changes in DMN neuronal connection and cerebellar regions in acute stage of mTBI patients can be an initial step of damages leading to cognitive deficit which can be developed in future.ΠΠ΅Π³ΠΊΠ°Ρ ΡΠ΅ΡΠ΅ΠΏΠ½ΠΎ-ΠΌΠΎΠ·Π³ΠΎΠ²Π°Ρ ΡΡΠ°Π²ΠΌΠ° (Π»Π§ΠΠ’) ΡΠ²Π»ΡΠ΅ΡΡΡ Π½Π°ΠΈΠ±ΠΎΠ»Π΅Π΅ ΡΠ°ΡΠΏΡΠΎΡΡΡΠ°Π½Π΅Π½Π½ΡΠΌ Π½Π΅Π²ΡΠΎΠ»ΠΎΠ³ΠΈΡΠ΅ΡΠΊΠΈΠΌ ΠΏΠΎΠ²ΡΠ΅ΠΆΠ΄Π΅Π½ΠΈΠ΅ΠΌ Ρ Π΄Π΅ΡΠ΅ΠΉ, ΠΏΠΎΡΡΠΎΠΌΡ ΡΡΠ΅Π·Π²ΡΡΠ°ΠΉΠ½ΠΎ Π²Π°ΠΆΠ½ΠΎ ΠΈΠ΄Π΅Π½ΡΠΈΡΠΈΡΠΈΡΠΎΠ²Π°ΡΡ ΠΈ ΠΏΡΠΎΠ°Π½Π°Π»ΠΈΠ·ΠΈΡΠΎΠ²Π°ΡΡ Π±ΠΈΠΎΠΌΠ°ΡΠΊΠ΅ΡΡ, ΠΊΠΎΡΠΎΡΡΠ΅ ΠΌΠΎΠ³ΡΡ ΠΏΠΎΠΌΠΎΡΡ Π² ΠΏΡΠΎΡΠ΅ΡΡΠ°Ρ
Π»Π΅ΡΠ΅Π½ΠΈΡ ΠΈ Π²ΡΠ·Π΄ΠΎΡΠΎΠ²Π»Π΅Π½ΠΈΡ ΠΏΠ°ΡΠΈΠ΅Π½ΡΠ° Ρ Π»Π§ΠΠ’.Π¦Π΅Π»Ρ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΡ: ΠΏΠΎΠ΄ΡΠ²Π΅ΡΠ΄ΠΈΡΡ Π³ΠΈΠΏΠΎΡΠ΅Π·Ρ ΠΎ ΡΠΎΠΌ, ΡΡΠΎ Π½Π°ΡΡΡΠ΅Π½ΠΈΡ ΡΡΠ½ΠΊΡΠΈΠΎΠ½Π°Π»ΡΠ½ΡΡ
ΡΠ²ΡΠ·Π΅ΠΉ ΠΌΠ΅ΠΆΠ΄Ρ Π½Π΅ΠΏΠΎΠ²ΡΠ΅ΠΆΠ΄Π΅Π½Π½ΡΠΌ ΠΌΠΎΠ·ΠΆΠ΅ΡΠΊΠΎΠΌ ΠΈ ΡΠ·Π»Π°ΠΌΠΈ ΡΠ΅ΡΠΈ DMN Π²ΠΊΠ»ΡΡΠ΅Π½Ρ Π² ΡΠΈΠΌΠΏΡΠΎΠΌΠ°ΡΠΈΡΠ΅ΡΠΊΠΎΠ΅ ΠΏΡΠΎΡΠ²Π»Π΅Π½ΠΈΠ΅ Π»Π§ΠΠ’.ΠΠ΅ΡΠΎΠ΄Ρ. ΠΠ±ΡΠ»Π΅Π΄ΠΎΠ²Π°Π½Ρ 28 ΠΠ -Π½Π΅Π³Π°ΡΠΈΠ²Π½ΡΡ
ΠΏΠ°ΡΠΈΠ΅Π½ΡΠΎΠ² Ρ Π»Π§ΠΠ’Π² Π²ΠΎΠ·ΡΠ°ΡΡΠ΅ ΠΎΡ 12 Π΄ΠΎ 17 Π»Π΅Ρ (ΡΡΠ΅Π΄Π½ΠΈΠΉ Π²ΠΎΠ·ΡΠ°ΡΡ 14,7 Π³ΠΎΠ΄Π°). ΠΠΎΠ½ΡΡΠΎΠ»ΡΠ½Π°Ρ Π³ΡΡΠΏΠΏΠ° ΡΠΎΡΡΠΎΡΠ»Π° ΠΈΠ· 23 Π·Π΄ΠΎΡΠΎΠ²ΡΡ
Π΄Π΅ΡΠ΅ΠΉ. ΠΡΠ΅ ΠΠ Π’-ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΡ ΠΏΡΠΎΠ²ΠΎΠ΄ΠΈΠ»ΠΈΡΡ Π½Π° ΡΠΊΠ°Π½Π΅ΡΠ΅ Philips Achieva dStream 3,0 TΠ», ΠΎΠ±ΠΎΡΡΠ΄ΠΎΠ²Π°Π½Π½ΠΎΠΌ 32-ΠΊΠ°Π½Π°Π»ΡΠ½ΠΎΠΉ Π³ΠΎΠ»ΠΎΠ²Π½ΠΎΠΉ ΠΊΠ°ΡΡΡΠΊΠΎΠΉ Philips dStream. ΠΡΠΎΠ²Π΅Π΄Π΅Π½Π° ΡΠΠ Π’ ΡΠΎΡΡΠΎΡΠ½ΠΈΡ ΠΏΠΎΠΊΠΎΡ (EPI ΠΏΠΎΡΠ»Π΅Π΄ΠΎΠ²Π°ΡΠ΅Π»ΡΠ½ΠΎΡΡΡ, TR = 3000 ΠΌΡ, Π²ΡΠ΅ΠΌΡ ΡΡ
Π° (TE) = 30 ΠΌΡ, 80 Π΄ΠΈΠ½Π°ΠΌΠΈΠΊΠΎΠ² Ρ Π΄ΠΈΠ½Π°ΠΌΠΈΡΠ΅ΡΠΊΠΈΠΌ Π²ΡΠ΅ΠΌΠ΅Π½Π΅ΠΌ ΡΠΊΠ°Π½ΠΈΡΠΎΠ²Π°Π½ΠΈΡ 3 Ρ). ΠΠ°Π½Π½ΡΠ΅ ΡΠΠ Π’ ΠΎΠ±ΡΠ°Π±ΠΎΡΠ°Π½Ρ Ρ ΠΈΡΠΏΠΎΠ»ΡΠ·ΠΎΠ²Π°Π½ΠΈΠ΅ΠΌ ΠΏΡΠΎΠ³ΡΠ°ΠΌΠΌΠ½ΠΎΠ³ΠΎ ΠΏΠ°ΠΊΠ΅ΡΠ° CONN.Π Π΅Π·ΡΠ»ΡΡΠ°ΡΡ. ΠΠ΅ ΠΎΠ±Π½Π°ΡΡΠΆΠ΅Π½ΠΎ ΡΡΠ°ΡΠΈΡΡΠΈΡΠ΅ΡΠΊΠΈ Π·Π½Π°ΡΠΈΠΌΠΎΠ³ΠΎ ΡΠ°Π·Π»ΠΈΡΠΈΡ Π² Π·Π½Π°ΡΠ΅Π½ΠΈΡΡ
ΠΊΠΎΡΡΡΠΈΡΠΈΠ΅Π½ΡΠΎΠ² ΡΡΠ½ΠΊΡΠΈΠΎΠ½Π°Π»ΡΠ½ΡΡ
ΡΠ²ΡΠ·Π΅ΠΉ ΠΌΠ΅ΠΆΠ΄Ρ ΠΎΠ±Π»Π°ΡΡΡΠΌΠΈ ΡΠ΅ΡΠΈ DMN Π² Π³ΡΡΠΏΠΏΠ°Ρ
ΠΏΠ°ΡΠΈΠ΅Π½ΡΠΎΠ² ΠΈ ΠΊΠΎΠ½ΡΡΠΎΠ»Ρ. ΠΠ΅ΠΆΠ³ΡΡΠΏΠΏΠΎΠ²ΠΎΠΉ Π°Π½Π°Π»ΠΈΠ· Π²ΡΡΠ²ΠΈΠ» ΡΡΠ°ΡΠΈΡΡΠΈΡΠ΅ΡΠΊΠΈ Π·Π½Π°ΡΠΈΠΌΠΎΠ΅ (Ρ < 0,05) ΡΠ°Π·Π»ΠΈΡΠΈΠ΅ Π² Π½Π΅ΠΉΡΠΎΠ½Π½ΡΡ
ΡΠ²ΡΠ·ΡΡ
ΠΌΠ΅ΠΆΠ΄Ρ ΡΠ°ΡΡΡΠΌΠΈ DMN ΠΈ ΡΠ΅ΡΠ²Π΅ΠΌ ΠΌΠΎΠ·ΠΆΠ΅ΡΠΊΠ° (vermis, ΡΡΡΡΠΊΡΡΡΠ½Π°Ρ ΡΠ°ΡΡΡ ΠΌΠΎΠ·ΠΆΠ΅ΡΠΊΠ°): ΠΏΠΎΠ»ΠΎΠΆΠΈΡΠ΅Π»ΡΠ½Π°Ρ ΡΠ²ΡΠ·Ρ Π² ΠΊΠΎΠ½ΡΡΠΎΠ»ΡΠ½ΠΎΠΉ Π³ΡΡΠΏΠΏΠ΅ ΠΈ ΠΎΡΡΠΈΡΠ°ΡΠ΅Π»ΡΠ½Π°Ρ ΡΠ²ΡΠ·Ρ Π² Π³ΡΡΠΏΠΏΠ΅ ΠΏΠ°ΡΠΈΠ΅Π½ΡΠΎΠ².ΠΠ°ΠΊΠ»ΡΡΠ΅Π½ΠΈΠ΅. ΠΡΡΠ²Π»Π΅Π½Π½ΡΠ΅ ΠΈΠ·ΠΌΠ΅Π½Π΅Π½ΠΈΡ Π² Π½Π΅ΠΉΡΠΎΠ½Π°Π»ΡΠ½ΡΡ
ΡΠ²ΡΠ·ΡΡ
ΠΌΠ΅ΠΆΠ΄Ρ ΠΎΠ±Π»Π°ΡΡΡΠΌΠΈ DMN ΠΈ ΠΌΠΎΠ·ΠΆΠ΅ΡΠΊΠ° Ρ ΠΏΠ°ΡΠΈΠ΅Π½ΡΠΎΠ² Ρ Π»Π§ΠΠ’ Π² ΠΎΡΡΡΠΎΠΌ ΠΏΠ΅ΡΠΈΠΎΠ΄Π΅ ΠΌΠΎΠ³ΡΡ Π±ΡΡΡ Π½Π°ΡΠ°Π»ΡΠ½ΡΠΌ ΡΡΠ°ΠΏΠΎΠΌ ΠΏΠΎΠ²ΡΠ΅ΠΆΠ΄Π΅Π½ΠΈΠΉ, ΠΏΡΠΈΠ²ΠΎΠ΄ΡΡΠΈΡ
ΠΊ ΠΊΠΎΠ³Π½ΠΈΡΠΈΠ²Π½ΠΎΠΌΡ Π΄Π΅ΡΠΈΡΠΈΡΡ, ΠΊΠΎΡΠΎΡΡΠΉ ΠΌΠΎΠΆΠ΅Ρ ΡΠ°Π·Π²ΠΈΡΡΡΡ Π² Π±ΡΠ΄ΡΡΠ΅ΠΌ
Π ΠΎΠ»Ρ ΠΌΠ°Π³Π½ΠΈΡΠ½ΠΎ-ΡΠ΅Π·ΠΎΠ½Π°Π½ΡΠ½ΠΎΠΉ ΡΠΎΠΌΠΎΠ³ΡΠ°ΡΠΈΠΈ ΠΏΡΠΈ ΠΎΡΡΡΠΎΠΉ ΡΡΠ°Π²ΠΌΠ΅ ΡΠ΅ΠΉΠ½ΠΎΠ³ΠΎ ΠΎΡΠ΄Π΅Π»Π° ΠΏΠΎΠ·Π²ΠΎΠ½ΠΎΡΠ½ΠΈΠΊΠ° Ρ Π΄Π΅ΡΠ΅ΠΉ
Aim. To evaluate the role of magnetic resonance imaging (MRI) as a diagnostic method in children with acute trauma of the cervical spine and spinal cord, to compare the correspondence of MRI results with neurologic symptoms in accordance with the ASIA scale.Materials and methods. 156 children with acute trauma of spine and spinal cord at the age from 6 months up to 18 years were studied. MRI was performed on a Phillips Achieva 3T scanner. The standard protocol included MYUR (myelography) in coronal and sagittal projections, STIR and T2VI FS SE in sagittal projection, T2VI SE or T2 * VI FSGE (axial projection), 3D T1VI FSGE before and after contrast enhancement. Contrast substance was injected intravenously in the form of a bolus at the rate of 0.1 mmol/kg (equivalent to 0.1 ml/kg) at a rate of 3 to 4 ml.Results. The causes of cervical spine blunt trauma were: road accidents (55), catatrauma (60), βdiverβ trauma (21), blunt trauma (20). Intramedullary lesions of the spinal cord were detected: concussion (49), bruising / crushing (27), hematomia (34), disruption with divergence of segments (21), accompanied by edema (141); extramedullary lesions: epi- and subdural, intralesive and sub-connective and soft tissues hematomas (68), ruptures of bundles (48), fractures (108), dislocation and subluxation of the vertebrae (35), traumatic disc herniation (37), spinal cord compression and/or rootlets (63), statics violation (134), instability (156).Conclusion. MRI is the optimal method for spinal cord injury diagnostics. In the acute period of injury this technique has limited application, but it can however serve as a primary diagnostic method in these patients. MRI should be performed no later than the first 72 hours after injury. The most optimal for visualization of cervical spine trauma and spinal cord are T2VI SE and STIR in sagittal projection with suppression of signal from fat. MRI results correlate with neurologic symptoms at the time of performance according to the ASIA scale, and therefore MRI should be performed in all patients with acute cervical spine trauma, whenever possible.Π¦Π΅Π»Ρ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΡ: ΠΎΡΠ΅Π½ΠΈΡΡ ΡΠΎΠ»Ρ ΠΌΠ°Π³Π½ΠΈΡΠ½ΠΎ-ΡΠ΅Π·ΠΎΠ½Π°Π½ΡΠ½ΠΎΠΉ ΡΠΎΠΌΠΎΠ³ΡΠ°ΡΠΈΠΈ (ΠΠ Π’) Π² ΠΊΠ°ΡΠ΅ΡΡΠ²Π΅ ΠΌΠ΅ΡΠΎΠ΄Π° Π΄ΠΈΠ°Π³Π½ΠΎΡΡΠΈΠΊΠΈ Ρ Π΄Π΅ΡΠ΅ΠΉ Ρ ΡΡΠ°Π²ΠΌΠΎΠΉ ΡΠ΅ΠΉΠ½ΠΎΠ³ΠΎ ΠΎΡΠ΄Π΅Π»Π° ΠΏΠΎΠ·Π²ΠΎΠ½ΠΎΡΠ½ΠΈΠΊΠ° ΠΈ ΡΠΏΠΈΠ½Π½ΠΎΠ³ΠΎ ΠΌΠΎΠ·Π³Π°, ΡΡΠ°Π²Π½ΠΈΡΡ ΡΠΎΠΎΡΠ²Π΅ΡΡΡΠ²ΠΈΠ΅ ΡΠ΅Π·ΡΠ»ΡΡΠ°ΡΠΎΠ² ΠΠ Π’ Ρ Π½Π΅Π²ΡΠΎΠ»ΠΎΠ³ΠΈΡΠ΅ΡΠΊΠΈΠΌΠΈ ΡΠΈΠΌΠΏΡΠΎΠΌΠ°ΠΌΠΈ ΠΈ ΡΠΊΠ°Π»ΠΎΠΉ ASIA.ΠΠ°ΡΠ΅ΡΠΈΠ°Π» ΠΈ ΠΌΠ΅ΡΠΎΠ΄Ρ. ΠΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΎ 156 Π΄Π΅ΡΠ΅ΠΉ Ρ ΠΎΡΡΡΠΎΠΉ ΡΡΠ°Π²ΠΌΠΎΠΉ ΠΏΠΎΠ·Π²ΠΎΠ½ΠΎΡΠ½ΠΈΠΊΠ° ΠΈ ΡΠΏΠΈΠ½Π½ΠΎΠ³ΠΎ ΠΌΠΎΠ·Π³Π° Π² Π²ΠΎΠ·ΡΠ°ΡΡΠ΅ ΠΎΡ 6 ΠΌΠ΅Ρ Π΄ΠΎ 18 Π»Π΅Ρ. ΠΠ Π’ ΠΏΡΠΎΠ²ΠΎΠ΄ΠΈΠ»Π°ΡΡ Π½Π° ΡΠΎΠΌΠΎΠ³ΡΠ°ΡΠ΅ Phillips Achieva 3 Π’Π». Π‘ΡΠ°Π½Π΄Π°ΡΡΠ½ΡΠΉ ΠΏΡΠΎΡΠΎΠΊΠΎΠ» ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΡ Π²ΠΊΠ»ΡΡΠ°Π»: ΠΌΠΈΠ΅Π»ΠΎΠ³ΡΠ°ΡΠΈΡ (MYUR) Π² ΠΊΠΎΡΠΎΠ½Π°ΡΠ½ΠΎΠΉ ΠΈ ΡΠ°Π³ΠΈΡΡΠ°Π»ΡΠ½ΠΎΠΉ ΠΏΡΠΎΠ΅ΠΊΡΠΈΡΡ
, STIR ΠΈ Π’2ΠΠ FS SE Π² ΡΠ°Π³ΠΈΡΡΠ°Π»ΡΠ½ΠΎΠΉ ΠΏΡΠΎΠ΅ΠΊΡΠΈΠΈ, Π’2ΠΠ SE ΠΈΠ»ΠΈ Π’2ΠΠ FSGE (Π°ΠΊΡΠΈΠ°Π»ΡΠ½Π°Ρ ΠΏΡΠΎΠ΅ΠΊΡΠΈΡ), 3D Π’1ΠΠ FSGE Π΄ΠΎ ΠΈ ΠΏΠΎΡΠ»Π΅ ΠΊΠΎΠ½ΡΡΠ°ΡΡΠ½ΠΎΠ³ΠΎ ΡΡΠΈΠ»Π΅Π½ΠΈΡ. ΠΠΎΠ½ΡΡΠ°ΡΡΠ½ΠΎΠ΅ Π²Π΅ΡΠ΅ΡΡΠ²ΠΎ Π²Π²ΠΎΠ΄ΠΈΠ»ΠΎΡΡ Π²Π½ΡΡΡΠΈΠ²Π΅Π½Π½ΠΎ Π² Π²ΠΈΠ΄Π΅ Π±ΠΎΠ»ΡΡΠ° ΠΈΠ· ΡΠ°ΡΡΠ΅ΡΠ° 0,1 ΠΌΠΌΠΎΠ»Ρ/ΠΊΠ³ (ΡΠΊΠ²ΠΈΠ²Π°Π»Π΅Π½ΡΠ½ΠΎ 0,1 ΠΌΠ»/ΠΊΠ³) ΡΠΎ ΡΠΊΠΎΡΠΎΡΡΡΡ 3β4 ΠΌΠ».Π Π΅Π·ΡΠ»ΡΡΠ°ΡΡ. ΠΡΠΈΡΠΈΠ½Π°ΠΌΠΈ ΡΡΠΏΠΎΠΉ ΡΡΠ°Π²ΠΌΡ ΡΠ΅ΠΉΠ½ΠΎΠ³ΠΎ ΠΎΡΠ΄Π΅Π»Π° ΠΏΠΎΠ·Π²ΠΎΠ½ΠΎΡΠ½ΠΈΠΊΠ° ΡΠ²ΠΈΠ»ΠΈΡΡ: Π΄ΠΎΡΠΎΠΆΠ½ΠΎ-ΡΡΠ°Π½ΡΠΏΠΎΡΡΠ½ΡΠ΅ ΠΏΡΠΎΠΈΡΡΠ΅ΡΡΠ²ΠΈΡ (55), ΠΊΠ°ΡΠ°ΡΡΠ°Π²ΠΌΠ° (60), ΡΡΠ°Π²ΠΌΠ° βΠ½ΡΡΡΠ»ΡΡΠΈΠΊΠ°β (21), ΡΡΠΏΠ°Ρ ΡΡΠ°Π²ΠΌΠ° (20). ΠΡΠ»ΠΈ Π²ΡΡΠ²Π»Π΅Π½Ρ ΠΈΠ½ΡΡΠ°ΠΌΠ΅Π΄ΡΠ»Π»ΡΡΠ½ΡΠ΅ ΠΏΠΎΠ²ΡΠ΅ΠΆΠ΄Π΅Π½ΠΈΡ ΡΠΏΠΈΠ½Π½ΠΎΠ³ΠΎ ΠΌΠΎΠ·Π³Π°: ΡΠΎΡΡΡΡΠ΅Π½ΠΈΠ΅ (49), ΡΡΠΈΠ±/ΡΠ°Π·ΠΌΠΎΠ·ΠΆΠ΅Π½ΠΈΠ΅ (27), Π³Π΅ΠΌΠ°ΡΠΎΠΌΠΈΠ΅Π»ΠΈΡ (34), ΡΠ°Π·ΡΡΠ² Ρ ΡΠ°ΡΡ
ΠΎΠΆΠ΄Π΅Π½ΠΈΠ΅ΠΌ ΠΎΡΡΠ΅Π·ΠΊΠΎΠ² (21), ΡΠΎΠΏΡΠΎΠ²ΠΎΠΆΠ΄Π°Π²ΡΠΈΠ΅ΡΡ ΠΎΡΠ΅ΠΊΠΎΠΌ (141); ΡΠΊΡΡΡΠ°ΠΌΠ΅Π΄ΡΠ»Π»ΡΡΠ½ΡΠ΅ ΠΏΠΎΠ²ΡΠ΅ΠΆΠ΄Π΅Π½ΠΈΡ: ΡΠΏΠΈΠΈ ΡΡΠ±Π΄ΡΡΠ°Π»ΡΠ½ΡΠ΅, Π²Π½ΡΡΡΠΈ- ΠΈ ΠΏΠΎΠ΄ΡΠ²ΡΠ·ΠΎΡΠ½ΡΠ΅ ΠΈ Π³Π΅ΠΌΠ°ΡΠΎΠΌΡ ΠΌΡΠ³ΠΊΠΈΡ
ΡΠΊΠ°Π½Π΅ΠΉ (68), ΡΠ°Π·ΡΡΠ²Ρ ΡΠ²ΡΠ·ΠΎΠΊ (48), ΠΏΠ΅ΡΠ΅Π»ΠΎΠΌΡ (108), Π²ΡΠ²ΠΈΡ
ΠΈ ΠΏΠΎΠ΄Π²ΡΠ²ΠΈΡ
ΠΏΠΎΠ·Π²ΠΎΠ½ΠΊΠΎΠ² (35), ΡΡΠ°Π²ΠΌΠ°ΡΠΈΡΠ΅ΡΠΊΠΈΠ΅ Π³ΡΡΠΆΠΈ Π΄ΠΈΡΠΊΠ° (37), ΠΊΠΎΠΌΠΏΡΠ΅ΡΡΠΈΡ ΡΠΏΠΈΠ½Π½ΠΎΠ³ΠΎ ΠΌΠΎΠ·Π³Π° ΠΈ/ΠΈΠ»ΠΈ ΠΊΠΎΡΠ΅ΡΠΊΠΎΠ² (63), Π½Π°ΡΡΡΠ΅Π½ΠΈΠ΅ ΡΡΠ°ΡΠΈΠΊΠΈ (134), Π½Π΅ΡΡΠ°Π±ΠΈΠ»ΡΠ½ΠΎΡΡΡ (156).ΠΠ°ΠΊΠ»ΡΡΠ΅Π½ΠΈΠ΅. ΠΠ Π’ β ΠΎΠΏΡΠΈΠΌΠ°Π»ΡΠ½ΡΠΉ ΠΌΠ΅ΡΠΎΠ΄ Π΄ΠΈΠ°Π³Π½ΠΎΡΡΠΈΠΊΠΈ ΠΏΠΎΠ·Π²ΠΎΠ½ΠΎΡΠ½ΠΎ-ΡΠΏΠΈΠ½Π½ΠΎΠΌΠΎΠ·Π³ΠΎΠ²ΠΎΠΉ ΡΡΠ°Π²ΠΌΡ. Π ΠΎΡΡΡΡΠΉ ΠΏΠ΅ΡΠΈΠΎΠ΄ ΡΡΠ°Π²ΠΌΡ ΠΎΠ½Π° ΠΈΠΌΠ΅Π΅Ρ ΠΎΠ³ΡΠ°Π½ΠΈΡΠ΅Π½Π½ΠΎΠ΅ ΠΏΡΠΈΠΌΠ΅Π½Π΅Π½ΠΈΠ΅, Π½ΠΎ ΠΎΠ΄Π½Π°ΠΊΠΎ ΠΌΠΎΠΆΠ΅Ρ ΡΠ»ΡΠΆΠΈΡΡ ΠΌΠ΅ΡΠΎΠ΄ΠΎΠΌ ΠΏΠ΅ΡΠ²ΠΈΡΠ½ΠΎΠΉ Π΄ΠΈΠ°Π³Π½ΠΎΡΡΠΈΠΊΠΈ Ρ ΡΡΠΈΡ
Π±ΠΎΠ»ΡΠ½ΡΡ
. ΠΠ Π’ ΠΆΠ΅Π»Π°ΡΠ΅Π»ΡΠ½ΠΎ Π²ΡΠΏΠΎΠ»Π½ΡΡΡ Π½Π΅ ΠΏΠΎΠ·Π΄Π½Π΅Π΅ ΠΏΠ΅ΡΠ²ΡΡ
72 Ρ ΠΏΠΎΡΠ»Π΅ ΡΡΠ°Π²ΠΌΡ. ΠΠ°ΠΈΠ±ΠΎΠ»Π΅Π΅ ΠΎΠΏΡΠΈΠΌΠ°Π»ΡΠ½ΡΠΌΠΈ Π΄Π»Ρ Π²ΠΈΠ·ΡΠ°Π»ΠΈΠ·Π°ΡΠΈΠΈ ΡΡΠ°Π²ΠΌΡ ΡΠ΅ΠΉΠ½ΠΎΠ³ΠΎ ΠΎΡΠ΄Π΅Π»Π° ΠΏΠΎΠ·Π²ΠΎΠ½ΠΎΡΠ½ΠΈΠΊΠ° ΠΈ ΡΠΏΠΈΠ½Π½ΠΎΠ³ΠΎ ΠΌΠΎΠ·Π³Π° ΡΠ²Π»ΡΡΡΡΡ Π’2ΠΠ SE ΠΈ STIR Π² ΡΠ°Π³ΠΈΡΡΠ°Π»ΡΠ½ΠΎΠΉ ΠΏΡΠΎΠ΅ΠΊΡΠΈΠΈ Ρ ΠΏΠΎΠ΄Π°Π²Π»Π΅Π½ΠΈΠ΅ΠΌ ΡΠΈΠ³Π½Π°Π»Π° ΠΎΡ ΠΆΠΈΡΠ°. Π Π΅Π·ΡΠ»ΡΡΠ°ΡΡ ΠΠ Π’ Π½Π° ΠΌΠΎΠΌΠ΅Π½Ρ Π²ΡΠΏΠΎΠ»Π½Π΅Π½ΠΈΡ ΠΊΠΎΡΡΠ΅Π»ΠΈΡΡΡΡ Ρ Π½Π΅Π²ΡΠΎΠ»ΠΎΠ³ΠΈΡΠ΅ΡΠΊΠΎΠΉ ΡΠΈΠΌΠΏΡΠΎΠΌΠ°ΡΠΈΠΊΠΎΠΉ Π² ΡΠΎΠΎΡΠ²Π΅ΡΡΡΠ²ΠΈΠΈ ΡΠΎ ΡΠΊΠ°Π»ΠΎΠΉ ASIA, Π° ΠΏΠΎΡΡΠΎΠΌΡ ΠΠ Π’ ΡΠ»Π΅Π΄ΡΠ΅Ρ ΠΏΡΠΎΠ²ΠΎΠ΄ΠΈΡΡ Ρ Π²ΡΠ΅Ρ
ΠΏΠ°ΡΠΈΠ΅Π½ΡΠΎΠ² Ρ ΠΎΡΡΡΠΎΠΉ ΡΡΠ°Π²ΠΌΠΎΠΉ ΡΠ΅ΠΉΠ½ΠΎΠ³ΠΎ ΠΎΡΠ΄Π΅Π»Π° ΠΏΠΎΠ·Π²ΠΎΠ½ΠΎΡΠ½ΠΈΠΊΠ°, ΠΊΠΎΠ³Π΄Π° ΡΡΠΎ Π²ΠΎΠ·ΠΌΠΎΠΆΠ½ΠΎ
National scientific conference with international participation Biological rehabilitation of disturbed lands
The 10th national scientific conference with international participation Biological Rehabilitation of Disturbed Lands was held in the city of Yekaterinburg on September 4β7, 2017. More than 180 participants attended the conference from various institutions of 39 Russian cities of Russia and 7 countries (Azerbaijan, Armenia, Belarus, Kazakhstan, Morocco, Turkey, and Ukraine). Participation in the conference of a wide range of researchers and specialists is an indicator that the problem of rehabilitation is not becoming obsolete, but, on the contrary, it is growing more urgent. This problem is among the priority tasks of many regions of Russia and foreign countries in which oil and gas production, various mining industries are developed and the transformation of natural landscapes into post-industrial ones takes place. These problems are discussed at the conference, which takes place every 5 years in Yekaterinburg. Thanks to an active exchange of experience between specialists from different countries and due to analysis and discussion of the results, the prospects of cooperation aimed at improving the ecological situation and rational use of natural resources in the industrialized regions are developing. The publications of proceedings of the conference are of great scientific and practical value for scientists and specialists dealing with the problem of rehabilitation and monitoring of disturbed lands. Evaluating the global character of the problems of the conference, an appeal was addressed to the Governments of the regions of the Russian Federation for targeted financing of basic research in industrial regions with a high concentration of disturbed lands. To protect public health and preserve the gene pool of animals and plants, the need of assessing the quality of products obtained in the regions that undergo biological rehabilitation is emphasized. The published collection of conference proceedings presents the results of the research of the last decade
The preliminary diffusion tensor imaging study of cerebral microstructure in the acute phase of brain concussion
Purpose of the study. Concussion does not cause any lesions available for visualization using computed tomography and magnetic resonance imaging. However, it can cause changes at the microstructural level, which can be detected by the diffusion-tensor imaging. The purpose of this study is to identify the effect of acute concussion on diffusion parameters in the corpus callosum, corticospinal tract, and thalamus in children.Patients and methods. Fractional anisotropy and the apparent diffusion coefficient were determined in 11 patients with a diagnosis of concussion (41 Β± 19 hours from the moment of injury) and in 11 healthy subjects. Philips Achieva dStream 3T magnetic resonance imager was used. Diffusion tensor imaging data were processed in the Philips Intellispace Portal program in the Fibertrack section.Results. Fractional diffusion anisotropy significantly increases and the apparent diffusion coefficient decreases in the thalamus of patients with concussion. In corpus callosum there is a growth trend in fractional anisotropy.Conclusion. The detected changes indicate the initial stage of cell edema in the thalamus caused by concussion. Diffusion-tensor imaging is the only magnetic resonance imaging method which may be sensitive to this pathology