168 research outputs found
Parameters of Hardening of Platinum-Palladium Alloys with Alloy Additions in View of Baushinger Effect
Color Effects Associated with the 1999 Microlensing Brightness Peaks in Gravitationally Lensed Quasar Q2237+0305
Photometry of the Q2237+0305gravitational lens in VRI spectral bands with the
1.5-m telescope of the high-altitude Maidanak observatory in 1995-2000 is
presented. Monitoring of Q2237+0305 in July-October 2000, made at nearly daily
basis, did not reveal rapid (night-to-night and intranight) variations of
brightness of the components during this time period. Rather slow changes of
magnitudes of the components were observed, such as 0.08 mag fading of B and C
components and 0.05 mag brightening of D in R band during July 23 - October 7,
2000. By good luck three nights in 1999 were almost at the time of the strong
brightness peak of image C, and approximately in the middle of the ascending
slope of the image A brightness peak. The C component was the most blue one in
the system in 1998 and 1999, having changed its (V-I) color from 0.56 mag to
0.12 mag since August 1997, while its brightness increased almost 1.2 mag
during this time period. The A component behaved similarly between August 1998
and August 2000, having become 0.47 mag brighter in R, and at the same time,
0.15 mag bluer. A correlation between the color variations and variations of
magnitudes of the components is demonstrated to be significant and reaches
0.75, with a regression line slope of 0.33. A color (V-I) vrs color (V-R) plot
shows the components settled in a cluster, stretched along a line with a slope
of 1.31. Both slopes are noticeably smaller than those expected if a standard
galactic interstellar reddening law were responsible for the differences
between the colors of images and their variations over time. We attribute the
brightness and color changes to microlensing of the quasar's structure, which
we conclude is more compact at shorter wavelengths, as predicted by most quasar
models featuring an energizing central source.Comment: 14 pages, 7 figures, LaTeX, submitted to A&
Time delays in PG1115+080: new estimates
We report new estimates of the time delays in the quadruple gravitationally
lensed quasar PG1115+080, obtained from the monitoring data in filter R with
the 1.5-m telescope at the Maidanak Mountain (Uzbekistan, Central Asia) in
2004-2006. The time delays are 16.4 days between images C and B, and 12 days
between C and A1+A2, with image C being leading for both pairs. The only known
estimates of the time delays in PG1115 are those based on observations by
Schechter et al. (1997) -- 23.7 and 9.4 days between images C and B, C and
A1+A2, respectively, as calculated by Schechter et al., and 25 and 13.3 days as
revised by Barkana (1997) for the same image components with the use of another
method. The new values of time delays in PG 1115+080 may be expected to provide
larger estimates of the Hubble constant thus decreasing a diversity between the
H_0 estimates taken from gravitationally lensed quasars and with other methods.Comment: 5 pages, 2 figures, Accepted for publication in MNRAS Letter
Π‘arbohydrate metabolism disorders and their outcomes in the long-term period in hospitalized patients with COVID-19
BACKGROUND: Diabetes mellitus (DM) is a predisposing factor for the development of many infectious complications. Numerous studies have demonstrated the association of hyperglycemia in patients having DM with a high risk of a more unfavorable course of COVID-19. However, hyperglycemia is often detected in patients with a COVID-19 not having anamnesis of DM. The following remains unclear: the etiological factors causing such disorders of carbohydrate metabolism, the persistence of these disorders and the characteristics of the course, as well as their comparative effect on the outcomes of COVID-19 and the further prognosis of patients.AIM: To study the prevalence and nature of carbohydrate metabolism disorders in patients with moderate to severe course of COVID-19, as well as 6 months after it.MATERIALS AND METHODS: Hospitalized patients with a confirmed diagnosis of COVID-19 of moderate and severe course of the disease were examined. There were no medical interventions outside recommendations of patient management. The observation was carried out during two time periods: inpatient treatment of a COVID-19 and 6 months after discharge. The following were evaluated: anamnesis data, the level of fasting plasma glucose; HbA1c, the results of computed tomography of the lungs, the drug therapy taken in all patients. Descriptive statistics methods were used to evaluate the parameters.RESULTS: The study included 280 patients with a median age of 61.5Β±14,2 years. During the disease, a violation ofΒ carbohydrate metabolism was detected in 188 people (67%), the remaining patients (33%) made up the normoglycemia group. Patients with hyperglycemia were stratified in a following way: a group with an established diagnosis of DM before COVID -19 included β 56 people (20%), a group with steroid-induced hyperglycemia (SIH) β 95 people (34%), a group of stress- induced hyperglycaemia β 20 people (7%), with undiagnosed diabetes β 17 people (6%). In the postcovid period (after 6 months), the normal level of glycemia in the same sample group was observed in 199 people (71.4%); 8 people (3%) were diagnosed with new cases of DM. The mortality rate was 10 people (3.6%) in the group of SIH (8 people) and undiagnosed DM (2 people).CONCLUSION: The use of glucocorticoids in hospitalized patients with COVID-19 leads to high incidence of SIH, which has reversible character. About 6% among hospitalized patients with a COVID-19 had undiagnosed DM and were not receiving antihyperglycemic therapy. The highest mortality was noted in the group of SIH, which allows us to conclude that SIH worsens the prognosis of patients to the greatest extent. Patients with newly diagnosed hyperglycemia, regardless of the level of hyperglycemia, are characterized by a more unfavorable course
Magnetic properties of colloidal suspensions of interacting magnetic particles
We review equilibrium thermodynamic properties of systems of magnetic
particles like ferrofluids in which dipolar interactions play an important
role. The review is focussed on two subjects: ({\em i}) the magnetization with
the initial magnetic susceptibility as a special case and ({\em ii}) the phase
transition behavior. Here the condensation ("gas/liquid") transition in the
subsystem of the suspended particles is treated as well as the
isotropic/ferromagnetic transition to a state with spontaneously generated
long--range magnetic order.Comment: Review. 62 pages, 4 figure
PG 1115+080: variations of the A2/A1 flux ratio and new values of the time delays
We report the results of our multicolor observations of PG 1115+080 with the
1.5-m telescope of the Maidanak Observatory (Uzbekistan, Central Asia) in
2001-2006. Monitoring data in filter R spanning the 2004, 2005 and 2006 seasons
(76 data points) demonstrate distinct brightness variations of the source
quasar with the total amplitude of almost 0.4 mag. Our R light curves have
shown image C leading B by 16.4d and image (A1+A2) by 12d that is inconsistent
with the previous estimates obtained by Schechter et al. in 1997 - 24.7d
between B and C and 9.4d between (A1+A2) and C. The new values of time delays
in PG 1115+080 must result in larger values for the Hubble constant, thus
reducing difference between its estimates taken from the gravitational lenses
and with other methods. Also, we analyzed variability of the A2/A1 flux ratio,
as well as color changes in the archetypal "fold" lens PG 1115+080. We found
the A1/A2 flux ratio to grow during 2001-2006 and to be larger at longer
wavelengths. In particular, the A2/A1 flux ratio reached 0.85 in filter I in
2006. We also present evidence that both the A1 and A2 images might have
undergone microlensing during 2001-2006, with the descending phase for A1 and
initial phase for A2. We find that the A2/A1 flux ratio anomaly in PG 1115 can
be well explained both by microlensing and by finite distance of the source
quasar from the caustic fold.Comment: 14 pages, 7 figures, 8 tables, Accepted for publication in MNRA
ΠΠ°Π±ΠΎΠ»Π΅Π²Π°Π΅ΠΌΠΎΡΡΡ ΡΠ°ΠΊΠΎΠΌ Π»Π΅Π³ΠΊΠΎΠ³ΠΎ Π² ΠΠΎΡΠΊΠΎΠ²ΡΠΊΠΎΠΉ ΠΎΠ±Π»Π°ΡΡΠΈ (1998β2018)
This review discusses the main statistical indicators for lung cancer (LC) in the Moscow region over the past 20 years from 1998 to 2018. Methods. The analysis of basic statistics was carried out on the basis of official statistics of the Moscow region in the period from 1998 to 2018. Results. A decrease in the incidence was revealed. The five-year survival rate increased. The morphological diagnostics of LC improved. The detection of the disease in the early stages improved. In addition, mortality has decreased, both overall, and one-year. Conclusion. The reduction of morbidity and mortality, as well as the improvement of early detection of patients with LC in the Moscow Region was facilitated by the introduction of tobacco control measures, the implementation of programs to fight cancer, improving the quality of diagnostics and improving the equipment of clinics and hospitals, as well as the use of new modern treatment methods, such targeted and immunotherapy.Π ΡΡΠ°ΡΡΠ΅ ΡΠ°ΡΡΠΌΠ°ΡΡΠΈΠ²Π°ΡΡΡΡ ΠΎΡΠ½ΠΎΠ²Π½ΡΠ΅ Π΄Π°Π½Π½ΡΠ΅ ΠΎΡΠΈΡΠΈΠ°Π»ΡΠ½ΠΎΠΉ ΡΡΠ°ΡΠΈΡΡΠΈΠΊΠΈ ΠΏΠΎ Π·Π°Π±ΠΎΠ»Π΅Π²Π°Π΅ΠΌΠΎΡΡΠΈ ΡΠ°ΠΊΠΎΠΌ Π»Π΅Π³ΠΊΠΎΠ³ΠΎ (Π Π) Π² ΠΠΎΡΠΊΠΎΠ²ΡΠΊΠΎΠΉ ΠΎΠ±Π»Π°ΡΡΠΈ Π·Π° ΠΏΠΎΡΠ»Π΅Π΄Π½ΠΈΠ΅ 20 Π»Π΅Ρ (1998β2018).ΠΠ°ΡΠ΅ΡΠΈΠ°Π»Ρ ΠΈ ΠΌΠ΅ΡΠΎΠ΄Ρ. ΠΡΠΎΠ²Π΅Π΄Π΅Π½ Π°Π½Π°Π»ΠΈΠ· (1998β2018).Π Π΅Π·ΡΠ»ΡΡΠ°ΡΡ. Π£ΡΡΠ°Π½ΠΎΠ²Π»Π΅Π½ΠΎ ΡΠ½ΠΈΠΆΠ΅Π½ΠΈΠ΅ ΠΏΠΎΠΊΠ°Π·Π°ΡΠ΅Π»Π΅ΠΉ Π·Π°Π±ΠΎΠ»Π΅Π²Π°Π΅ΠΌΠΎΡΡΠΈ ΠΈ ΡΠ²Π΅Π»ΠΈΡΠ΅Π½ΠΈΠ΅ 5-Π»Π΅ΡΠ½Π΅ΠΉ Π²ΡΠΆΠΈΠ²Π°Π΅ΠΌΠΎΡΡΠΈ. Π£Π»ΡΡΡΠΈΠ»ΠΈΡΡ ΠΏΠΎΠΊΠ°Π·Π°ΡΠ΅Π»ΠΈ ΠΌΠΎΡΡΠΎΠ»ΠΎΠ³ΠΈΡΠ΅ΡΠΊΠΎΠΉ Π΄ΠΈΠ°Π³Π½ΠΎΡΡΠΈΠΊΠΈ Π Π ΠΈ Π²ΡΡΠ²Π»ΡΠ΅ΠΌΠΎΡΡΠΈ Π·Π°Π±ΠΎΠ»Π΅Π²Π°Π½ΠΈΡ Π½Π° ΡΠ°Π½Π½ΠΈΡ
ΡΡΠ°Π΄ΠΈΡΡ
. ΠΠΎΠΊΠ°Π·Π°Π½ΠΎ ΡΠ½ΠΈΠΆΠ΅Π½ΠΈΠ΅ ΠΊΠ°ΠΊ ΠΎΠ±ΡΠ΅ΠΉ, ΡΠ°ΠΊ ΠΈ ΠΎΠ΄Π½ΠΎΠ³ΠΎΠ΄ΠΈΡΠ½ΠΎΠΉ Π»Π΅ΡΠ°Π»ΡΠ½ΠΎΡΡΠΈ.ΠΠ°ΠΊΠ»ΡΡΠ΅Π½ΠΈΠ΅. Π‘Π½ΠΈΠΆΠ΅Π½ΠΈΡ Π·Π°Π±ΠΎΠ»Π΅Π²Π°Π΅ΠΌΠΎΡΡΠΈ ΠΈ Π»Π΅ΡΠ°Π»ΡΠ½ΠΎΡΡΠΈ, Π° ΡΠ°ΠΊΠΆΠ΅ ΡΠ»ΡΡΡΠ΅Π½ΠΈΡ Π²ΡΡΠ²Π»ΡΠ΅ΠΌΠΎΡΡΠΈ Π±ΠΎΠ»ΡΠ½ΡΡ
Π Π Π½Π° ΡΠ°Π½Π½ΠΈΡ
ΡΡΠ°Π΄ΠΈΡΡ
Π² ΠΠΎΡΠΊΠΎΠ²ΡΠΊΠΎΠΉ ΠΎΠ±Π»Π°ΡΡΠΈ ΡΠΏΠΎΡΠΎΠ±ΡΡΠ²ΠΎΠ²Π°Π»ΠΎ Π²Π²Π΅Π΄Π΅Π½ΠΈΠ΅ ΠΏΡΠΎΡΠΈΠ²ΠΎΡΠ°Π±Π°ΡΠ½ΡΡ
ΠΌΠ΅Ρ, ΡΠ΅Π°Π»ΠΈΠ·Π°ΡΠΈΡ ΠΏΡΠΎΠ³ΡΠ°ΠΌΠΌ ΠΏΠΎ Π±ΠΎΡΡΠ±Π΅ Ρ ΠΎΠ½ΠΊΠΎΠ»ΠΎΠ³ΠΈΡΠ΅ΡΠΊΠΈΠΌΠΈ Π·Π°Π±ΠΎΠ»Π΅Π²Π°Π½ΠΈΡΠΌΠΈ, ΡΠ»ΡΡΡΠ΅Π½ΠΈΠ΅ ΠΊΠ°ΡΠ΅ΡΡΠ²Π° Π΄ΠΈΠ°Π³Π½ΠΎΡΡΠΈΠΊΠΈ ΠΈ ΠΎΡΠ½Π°ΡΠ΅Π½ΠΈΡ ΠΏΠΎΠ»ΠΈΠΊΠ»ΠΈΠ½ΠΈΠΊ ΠΈ ΡΡΠ°ΡΠΈΠΎΠ½Π°ΡΠΎΠ², Π° ΡΠ°ΠΊΠΆΠ΅ ΠΏΡΠΈΠΌΠ΅Π½Π΅Π½ΠΈΠ΅ Π½ΠΎΠ²ΡΡ
ΡΠΎΠ²ΡΠ΅ΠΌΠ΅Π½Π½ΡΡ
ΠΌΠ΅ΡΠΎΠ΄ΠΎΠ² ΡΠ΅ΡΠ°ΠΏΠΈΠΈ, Π² ΡΠ°ΡΡΠ½ΠΎΡΡΠΈ, ΡΠ°ΡΠ³Π΅ΡΠ½ΠΎΠΉ ΠΈ ΠΈΠΌΠΌΡΠ½ΠΎΡΠ΅ΡΠ°ΠΏΠΈΠΈ
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