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Relevant bibliographies by topics / Almost semi- Strong CJ- space

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Academic literature on the topic 'Almost semi- Strong CJ- space'

Author: Grafiati

Published: 3 June 2025

Last updated: 31 July 2025

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Journal articles on the topic "Almost semi- Strong CJ- space"

1

Akyol, M. A., and Y. Gündüzalp. "Pointwise semi-slant Riemannian maps into almost Hermitian manifolds and Casorati inequalities." Ukrains’kyi Matematychnyi Zhurnal 76, no. 9 (2024): 1271–90. http://dx.doi.org/10.3842/umzh.v76i9.7652.

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UDC 514 As a natural generalization of slant submanifolds [B.-Y. Chen, <em>Bull. Austral. Math. Soc.,</em> <strong>41</strong>, No. 1, 135 (1990)], slant submersions [B. Şahin, <em>Bull. Math. Soc. Sci. Math. Roumanie (N.S.),</em> <strong>54</strong>, No. 102, 93 (2011)], slant Riemannian maps [B. Şahin, <em>Quaestion. Math.,</em> <strong>36</strong>, No. 3, 449 (2013) and Int. J. <em>Geom. Methods Mod. Phys.,</em> <strong>10</strong>, Article 1250080 (2013)], pointwise slant submanifolds [B.-Y. Che

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Gómez-Garrido, M., V. Bujarrabal, J. Alcolea, R. Soria-Ruiz, P. de Vicente, and J. F. Desmurs. "Very fast variations of SiO maser emission in evolved stars." Astronomy & Astrophysics 642 (October 2020): A213. http://dx.doi.org/10.1051/0004-6361/202037499.

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Context. Stars on the asymptotic giant branch (AGB) are long-period variables that present strong flux variations at almost all wavelengths, including the SiO maser lines. The periods of these variations are of 300–500 days in Mira-type stars and somewhat shorter in semi-regular variables. The variability of the SiO lines on short timescales has been investigated, but the data are inconclusive. Aims. We aim to study the time evolution of the SiO maser lines in Mira-type and semi-regular variables at short timescales. We also discuss the origin of the observed fast variations. Methods. We obser

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Gagui, Abdelmalek. "Local linear estimation of a conditional hazard function under random censorship: strong consistency with convergence rates." STUDIES IN ENGINEERING AND EXACT SCIENCES 5, no. 2 (2024): e12245. https://doi.org/10.54021/seesv5n2-800.

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This paper explores the estimation of a conditional hazard function for a scalar response variable conditioned on a random predictor within a semi-metric space. Utilizing a local linear estimator, we address the challenges posed by censored and -mixing dependent data. The proposed method combines nonparametric functional data analysis techniques to estimate the conditional density and cumulative distribution functions. We establish almost sure convergence rates under specific regularity conditions, contributing to the theoretical understanding of hazard function estimation in complex data stru

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Lagos, Claudia del P., Aaron S. G. Robotham, James W. Trayford, et al. "From the far-ultraviolet to the far-infrared – galaxy emission at 0 ≤ z ≤ 10 in the shark semi-analytic model." Monthly Notices of the Royal Astronomical Society 489, no. 3 (2019): 4196–216. http://dx.doi.org/10.1093/mnras/stz2427.

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ABSTRACT We combine the shark semi-analytic model of galaxy formation with the prospect software tool for spectral energy distribution (SED) generation to study the multiwavelength emission of galaxies from the far-ultraviolet (FUV) to the far-infrared (FIR) at 0 ≤ z ≤ 10. We produce a physical model for the attenuation of galaxies across cosmic time by combining a local Universe empirical relation to compute the dust mass of galaxies from their gas metallicity and mass, attenuation curves derived from radiative transfer calculations of galaxies in the eagle hydrodynamic simulation suite, and

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Providence, Kevin Antonio. "Advancing The Blue Economy Through Sustainable Mariculture: The Prospect of Pearl Oyster and Sponge Cultivation in St. Vincent and The Grenadines." Gulf and Caribbean Research 35 (2024): 43–56. http://dx.doi.org/10.18785/gcr.3501.13.

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The Blue Economy is estimated to be worth over USD 2.5 trillion annually, or almost 3% of the world’s GDP in 2020. St. Vincent and the Grenadines (SVG) in the Caribbean region has a vast and rich marine space that is underutilized. This study aimed to explore the feasibility of pearl oyster and sponge farming to advance the country’s Blue Economy through sustainable mariculture. A qualitative approach was applied, using a literature review and thematic analysis of data gathered through semi—structured interviews and focus group discussions with relevant stakeholders. Among several species eval

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Lühr, H., and C. Manoj. "The complete spectrum of the equatorial electrojet related to solar tides: CHAMP observations." Annales Geophysicae 31, no. 8 (2013): 1315–31. http://dx.doi.org/10.5194/angeo-31-1315-2013.

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Abstract. Based on 10 yr of magnetic field measurements by the CHAMP satellite we draw a detailed picture of the equatorial electrojet (EEJ) tidal variations. For the first time the complete EEJ spectrum related to average solar tides has been compiled. A large fraction of the resulting spectrum is related to the switch on/off of the EEJ between day and night. This effect has carefully been considered when interpreting the results. As expected, largest amplitudes are caused by the migrating tides representing the mean diurnal variation. Higher harmonics of the daily variations show a 1/f fall-

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Lagache, G., M. Cousin та M. Chatzikos. "The [CII] 158 μm line emission in high-redshift galaxies". Astronomy & Astrophysics 609 (січень 2018): A130. http://dx.doi.org/10.1051/0004-6361/201732019.

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Gas is a crucial component of galaxies, providing the fuel to form stars, and it is impossible to understand the evolution of galaxies without knowing their gas properties. The [CII] fine structure transition at 158 μm is the dominant cooling line of cool interstellar gas, and is the brightest of emission lines from star forming galaxies from FIR through metre wavelengths, almost unaffected by attenuation. With the advent of ALMA and NOEMA, capable of detecting [CII]-line emission in high-redshift galaxies, there has been a growing interest in using the [CII] line as a probe of the physical co

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Heller, R., and R. Barnes. "Runaway greenhouse effect on exomoons due to irradiation from hot, young giant planets." International Journal of Astrobiology 14, no. 2 (2014): 335–43. http://dx.doi.org/10.1017/s1473550413000463.

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AbstractThe Kepler space telescope has proven capable of detecting transits of objects almost as small as the Earth's Moon. Some studies suggest that moons as small as 0.2 Earth masses can be detected in the Kepler data by transit timing variations and transit duration variations of their host planets. If such massive moons exist around giant planets in the stellar habitable zone (HZ), then they could serve as habitats for extraterrestrial life. While earlier studies on exomoon habitability assumed the host planet to be in thermal equilibrium with the absorbed stellar flux, we here extend this

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Cámara, Fernando, Dan Holtstam, Nils Jansson, et al. "Zinkgruvanite, Ba<sub>4</sub>Mn<sup>2+</sup><sub>4</sub>Fe<sup>3+</sup><sub>2</sub>(Si<sub>2</sub>O<sub>7</sub>)<sub>2</sub>(SO<sub>4</sub>)<sub>2</sub>O<sub>2</sub>(OH)<sub>2</sub>, a new ericssonite-group mineral from the Zinkgruvan Zn-Pb-Ag-Cu deposit, Askersund, Örebro County, Sweden." European Journal of Mineralogy 33, no. 6 (2021): 659–73. http://dx.doi.org/10.5194/ejm-33-659-2021.

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Abstract. Zinkgruvanite, ideally Ba4Mn42+Fe23+(Si2O7)2(SO4)2O2(OH)2, is a new member of the ericssonite group, found in Ba-rich drill core samples from a sphalerite- and galena- and diopside-rich metatuffite succession from the Zinkgruvan mine, Örebro County, Sweden. Zinkgruvanite is associated with massive baryte, barytocalcite, diopside and minor witherite, cerchiaraite-Al, and sulfide minerals. It occurs as subhedral to euhedral flattened and elongated crystals up to 4 mm. It is almost black and semi-opaque with a dark-brown streak. The lustre is vitreous to sub-adamantine on crystal faces

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Jernyei Kiss, János. "„A bérc vadászkalandora.” Strobl Alajos budavári Mátyás-kútja." Művészettörténeti Értesítő 72, no. 2 (2025): 239–68. https://doi.org/10.1556/080.2023.00013.

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The Matthias Fountain is the main attraction in the Hunyadi Courtyard of the Royal Palace in Buda Castle. From the beginning, its creators wanted to evoke the figure of the great ruler, closely linked to the castle’s historical past, and at the same time to “capture a scene from the life of this gallant and popular king”. The theme chosen for Alajos Strobl’s work was Matthias’ hunting and romance in the Vértes Mountains, the story of Beautiful Ilonka, perpetuated by Mihály Vörösmarty’s poem. Its predecessor was an earlier ornamental fountain Miklós József Esterházy had commissioned for the cou

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