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Gotowe bibliografie tematyczne / CygX-2

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Gotowa bibliografia na temat „CygX-2”

Autor: Grafiati

Data publikacji: 2 czerwca 2025

Data aktualizacji: 31 lipca 2025

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Artykuły w czasopismach na temat "CygX-2"

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Jusman, Sri W. A., Febriana C. Iswanti, Franciscus D. Suyatna, Frans Ferdinal, Septelia I. Wanandi та Mohamad Sadikin. "Cytoglobin expression in oxidative stressed liver during systemic chronic normobaric hypoxia and relation with HIF-1α". Medical Journal of Indonesia 23, № 3 (2014): 133–8. http://dx.doi.org/10.13181/mji.v23i3.1025.

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Background: Liver is sensitive against hypoxia and hypoxia will stabilize HIF-1α. At the same time, hypoxia will produce reactive oxygen species (ROS) which can be scavenged by Cygb. The purpose of our study is to know, if normobaric hypoxia can induce Cygb expression and its association with HIF-1α stabilization.Methods: This is an experimental study using 28 male Sprague-Dawley rats, 150-200 g weight. Rats are divided into 7 groups: control group and treatment groups that are kept in hypoxic chamber (10% O2: 90% N2) for 6 hours, 1, 2, 3, 7 and 14 days. All rats are euthanized after treatment

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Mimura, Imari, Masaomi Nangaku, Hiroshi Nishi, Reiko Inagi, Tetsuhiro Tanaka, and Toshiro Fujita. "Cytoglobin, a novel globin, plays an antifibrotic role in the kidney." American Journal of Physiology-Renal Physiology 299, no. 5 (2010): F1120—F1133. http://dx.doi.org/10.1152/ajprenal.00145.2010.

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Cytoglobin (Cygb), a novel member of the globin superfamily, is expressed by fibroblasts in various organs. However, its function remains unknown. Because of its localization, we speculated that a biological role of Cygb may be related to fibrogenesis. To clarify the role of Cygb in kidney fibrosis, we employed the remnant kidney model in rats. Immunohistochemical analysis showed an increase in Cygb expression in parallel with disease progression. To investigate the functional consequence of Cygb upregulation, we established transgenic rats overexpressing rat Cygb. Overexpression of Cygb impro

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3

Kiss, L. L., N. Gőgh, J. Vinkó, et al. "Nova Cygni 2001/2 = V2275 Cyg." Astronomy & Astrophysics 384, no. 3 (2002): 982–86. http://dx.doi.org/10.1051/0004-6361:20020064.

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Yang, Chloe, Mina Dehghani, Wilma Hopman, and Sita D. Bhella. "Are We Choosing Mobilization Regimens for Autologous Stem Cell Transplantation in Multiple Myeloma Wisely?: A Single Centre Comparison of GCSF+/-Plerixafor Vs Cyclophosphamide/GCSF+/- Plerixafor." Blood 134, Supplement_1 (2019): 2136. http://dx.doi.org/10.1182/blood-2019-128819.

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Background: Autologous stem cell transplantation (ASCT) as consolidation post induction is standard of care for eligible multiple myeloma patients. Multiple strategies are employed for mobilization of stem cells in ASCT. Cyclophosphamide/GCSF is an effective standard regimen. However there are reported toxicities associated with cyclophosphamide including risk of febrile neutropenia. Since plerixafor was introduced in Canada, this mobilization agent has been increasingly used as needed with GCSF at Kingston Health Science Centre (KHSC), with elimination of cyclophosphamide. There is however hi

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Done, C., P. T. Z˙ycki, and D. A. Smith. "The X-ray spectrum of Cyg X-2." Monthly Notices of the Royal Astronomical Society 331, no. 2 (2002): 453–62. http://dx.doi.org/10.1046/j.1365-8711.2002.05195.x.

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Kuulkers, E., and M. van Der Klis. "Cyg X-2: Its Recurrent X-Ray Behaviour." International Astronomical Union Colloquium 158 (1996): 363–64. http://dx.doi.org/10.1017/s0252921100039130.

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Chiappetti, L., A. L. Ciapi, L. Maraschi, L. Stella, E. G. Tanzi, and A. Treves. "Exosat medium energy observations of Cyg X-2." Astrophysics and Space Science 131, no. 1-2 (1987): 691–95. http://dx.doi.org/10.1007/bf00668160.

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Hasinger, G., A. Langmeier, W. Pietsch, and M. Sztajno. "EXOSAT medium energy observations of Cyg X-2." Space Science Reviews 40, no. 1-2 (1985): 233–38. http://dx.doi.org/10.1007/bf00212891.

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Sazonov, A. N. "WBVR observations of the X-ray star V1341 Cyg = Cyg X-2 in 1986–1992." Astronomy Reports 55, no. 2 (2011): 142–58. http://dx.doi.org/10.1134/s1063772910121017.

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Farrukh, L., M. Felix, A. Ibrahim, R. Peredo-Wende, D. Jourd’heuil, and F. Jourd’heuil. "AB0755 INVESTIGATING CYTOGLOBIN IN GIANT CELL ARTERITIS: ITS ROLE IN THE PATHOGENESIS AND POTENTIAL AS A BIOMARKER." Annals of the Rheumatic Diseases 82, Suppl 1 (2023): 1584.2–1584. http://dx.doi.org/10.1136/annrheumdis-2023-eular.358.

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BackgroundCytoglobin (CYBG) is a non-erythroid globin that is found in medial smooth muscle cells (SMCs) of human vessels. Recent studies have postulated that CYGB act as a pro-survival factor during conditions associated with increased oxidative stress, by upregulating anti-apoptotic factors and antioxidant pathways. In this study, we hypothesized that CYGB regulates the inflammatory and antioxidant response associated with GCA pathogenesis.ObjectivesThe purpose of this study is to evaluate giant cell arteritis (GCA) vascular lesions for the expression of CYGB and its association with specifi

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Części książek na temat "CygX-2"

1

Kuulkers, E., and M. Van Der Klis. "Cyg X-2: its Recurrent X-ray Behaviour." In Cataclysmic Variables and Related Objects. Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0325-8_109.

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Hasinger, G., A. Langmeier, W. Pietsch, and M. Sztajno. "Exosat Medium Energy Observations of Cyg X-2." In X-Ray Astronomy in the Exosat Era. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5448-9_31.

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Hasinger, Günther. "Observations of Quasi-Periodic Oscillations in CYG X-2." In The Origin and Evolution of Neutron Stars. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-3913-4_65.

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Chiappetti, L., A. L. Ciapi, L. Maraschi, L. Stella, E. G. Tanzi, and A. Treves. "Exosat Medium Energy Observations of CYG X-2.: Spectra and QPOs." In Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-3801-4_99.

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Hasinger, G. "Quasi-Periodic Oscillations in the X-Ray Flux of CYG X-2 and their Relation to the Source Spectra." In The Evolution of Galactic X-Ray Binaries. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4594-4_11.

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Streszczenia konferencji na temat "CygX-2"

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Shirai, Hirohisa. "Soft X-ray emission from the Low Mass X-ray Binary Cyg X-2." In VII Microquasar Workshop: Microquasars and Beyond. Sissa Medialab, 2009. http://dx.doi.org/10.22323/1.062.0098.

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Shaposhnikov, I. "Wolf–Rayet stars mass-loss rates determined from spectroscopic measurements of the orbital evolution for close WR+OB binary systems." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.087.

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The most reliable method for estimating the rate of mass-loss by the Wolf–Rayet stars wind is based on the assessment of secular variations in the orbital periods for close binary systems containing such stars, most often WR+OB systems. Previously, almost only photometric observations of well-studied eclipsing close WR+OB binaries were used for these purposes. This report describes the results of the work on the search for mass-loss-induced evolutionary variations in the orbital period for close WR+OB binaries and the mass-loss rates measurements for WR stars in these systems. Orbital period v

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3

Ibrahimov, M. "Exotic red flares on stars as the observational manifestation of the asteroids in exoplanet systems." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.133.

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The published data on exotic red flares (RFs) obtained using optical/IR photometry was for the first time gathered and discussed in this paper. To date, the RFs have been observed: (a) in IR space missions (1–2 yr long IR brightening observed using WISE/NEOWISE and Spitzer in NGC 2547-ID8, HD 166191, WD 0145+234, and some others systems); (b) in five optical systems with the normal stars (UU CrB, AZ Ori, FF Ori, IX Oph, CU Cnc; three of the five systems are binaries; seven single flares were observed in 1980–2009 having a 1-hour average duration, an amplitude up to $2^{\rm m}$, and an energy u

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Trushkin, S., A. Shevchenko, N. Bursov, P. Tsybulev, and N. Nizhelsky. "Long-term multi-frequency studies of flaring activity from microquasars." In ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES. Proceedings of the VAK-2021 conference, Aug 23–28, 2021. Crossref, 2022. http://dx.doi.org/10.51194/vak2021.2022.1.1.196.

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The long-term monitoring at RATAN-600 of studies of bright X-ray binary stars in various ranges of the electromagneticspectrum, a search and detailed study of correlations between variable X-ray, radio and gamma radiation was carried out.It is a key point for understanding the formation of jet emissions from accreting matter onto a black hole (or neutron star).From April 2019 For a year, we began to use the multi-azimuth measurement mode on the Southern Sector antenna systemwith a ﬂat reﬂector, when 31 measurements of ﬂux densities at frequencies 4.7, 8.6, 15 and 30 GHz of several giant Cygnus

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