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61
Power Splitting Characteristic of Star Gearing based on Deformation Compatibility
Published 2016-01-01“…The deformation compatibility equations and the torque balance equations of a star gearing with three branches are estabished based on the characteristic that the system composes a closed-loop of power flow.In consideration of the parts manufacturing errors,assembly errors,bearing stiffness and float,the power splitting coefficient of each star gear and the system are calculated by using the theory of equivalent mesh error.The relation between the errors,float and the bearing stiffness and power splitting are analyzed from the perspective of statics,and comparing with planetary transmission.A new algorithm is proposed,the reference for the engineering application is provided.…”
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62
GRB 130603B: No Compelling Evidence for Neutron Star Merger
Published 2015-01-01“…Moreover, SHB plus a kilonova can be produced also by the collapse of a compact star (neutron star, strange star, or quark star) to a more compact object due to cooling, loss of angular momentum, or mass accretion.…”
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63
'Cranberry Star' - A New University of Florida Caladium Variety
Published 2009-01-01“…ENH1105/EP369: 'Cranberry Star' Caladium (ufl.edu) …”
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64
From Stars to Stones: The Cultural and Linguistic Roots of the Name ‘Skardu’
Published 2024-08-01Subjects: “…Toponymy, Etymology, Linguistic, Cultural, Star, Skardu, Tibetan, Balti…”
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65
Formation of Stripped Stars from Stellar Collisions in Galactic Nuclei
Published 2025-01-01“…TDEs of these stripped stars may therefore exhibit even more extreme nitrogen enhancement. …”
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66
'Cranberry Star' - A New University of Florida Caladium Variety
Published 2009-01-01“…ENH1105/EP369: 'Cranberry Star' Caladium (ufl.edu) …”
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67
Stability of compact stars in a uniform density background cloud
Published 2024-12-01“…Abstract We are discussing a scenario where a compact star (neutron star, NS) is embedded in a thin, uniform density background cloud (a remnant cloud after a supernova or a cloud generated from the late stages of a star e.g., a planetary nebula or asymptotic red giant phases) and its effect on the stability of the compact star. …”
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68
TELEVİZYON PROGRAMLARINDA ÜRÜN YERLEŞTİRME: “SURVİVOR ALL STAR” ÖRNEĞİ
Published 2017-01-01Subjects: Get full text
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69
Star Identification Algorithm Based on Dynamic Distance Ratio Matching
Published 2024-12-01Subjects: “…star tracker…”
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70
Revisiting the 3α reaction rates in helium burning stars
Published 2025-01-01“…This may be crucial for the early dynamics of helium burning stars.…”
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71
Hankel Determinants for the Logarithmic Coefficients of a Subclass of Close-to-Star Functions
Published 2024-01-01“…Suppose that ST1 is a class of close-to-star functions. In this paper, we investigated the estimate of Zalcman functional on the logarithmic coefficients and the third Hankel determinant for the class ST1 with the determinant entry of logarithmic coefficients. …”
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72
Hierarchical Classification of Variable Stars Using Deep Convolutional Neural Networks
Published 2022-04-01Subjects: “…variable stars…”
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73
Multicolor Ramsey numbers and star-critical Ramsey numbers involving fans
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74
Research on Load Characteristic of Star Gear Transmission System of Turbofan Engine
Published 2021-06-01“…A gear rotor bearing coupling dynamics model is established for the star gear transmission system of geared turbofan engine(GTF). …”
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75
Effect of Generalized Uncertainty Principle on Main-Sequence Stars and White Dwarfs
Published 2015-01-01“…Astrophysical objects such as main-sequence stars and white dwarfs are examined and discussed as an application. …”
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76
The Main Ionization Sources of Gas in Several Nearby Star Forming Galaxies
Published 2021-03-01“…In intermediate cases, when the contributions of radiation from OB stars and from shock waves mix, the identification becomes uncertain. …”
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77
Analysis of the Conformally Flat Approximation for Binary Neutron Star Initial Conditions
Published 2017-01-01“…The spatially conformally flat approximation (CFA) is a viable method to deduce initial conditions for the subsequent evolution of binary neutron stars employing the full Einstein equations. Here we analyze the viability of the CFA for the general relativistic hydrodynamic initial conditions of binary neutron stars. …”
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78
The Fault in our Stars – Starry-coloured Halos in Occipital Lobe Infarct
Published 2024-12-01“…She also complained of seeing multi-coloured rings in a star pattern, each episode lasting for 10 to 15 min. …”
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79
Can Effects of a Generalized Uncertainty Principle Appear in Compact Stars?
Published 2024-12-01“…The corresponding results for the equation of state and the mass-radius relation for neutron stars are in tune with recent observations with a maximum mass around 2.5 M<sub>⊙</sub> and radius close to 12 km. …”
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80
Thermal and Mechanical Properties of Biodegradable Star-Shaped/Linear Polylactide Stereocomplexes
Published 2015-01-01“…The 6-arm star-shaped poly(L-lactide) (6PLL)/linear poly(D-lactide) (1PDL) stereocomplex films were prepared by the solvent casting method. …”
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