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701
Comparison study of bioelectrical impedance analyzers for measuring lower limb muscle mass in middle-aged and elderly adults
Published 2025-02-01“…The correlation coefficients of StarBIA201, BC418, InBody270, MC780, and InBody770 with DXA were 0.902, 0.903, 0.917, 0.925, and 0.928, respectively. …”
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702
Mesenchymal Stromal Cells: Novel Methods for Characterization, Understanding Differentiation, and Function
Published 2014-01-01Get full text
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703
The Natural Science Underlying Big History
Published 2014-01-01“…Nature’s many varied complex systems—including galaxies, stars, planets, life, and society—are islands of order within the increasingly disordered Universe. …”
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704
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705
Illicium floridanum Florida Anise Tree, Florida Anise
Published 2007-05-01“…It describes the plant’s physical characteristics, including its olive green leaves, reddish-purple flowers, and star-shaped seed pods. The document outlines the plant’s growth habits, preferred growing conditions, and uses in landscaping. …”
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706
Comparison of the Dynamic Balance in Youth Male Wrestlers According to Age, Body Mass Index, and Participation Level
Published 2021-08-01“…They were subdivided according to participation levels (elite and sub-elite), age (13-14,15-16,17-18) and BMI (25). The modified star excursion balance test (mSEBT) was performed by the same sports medicine specialist. …”
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707
Non-linear bi-algebraic curves and surfaces in moduli spaces of Abelian differentials
Published 2023-11-01“…Partly inspired by the case of homogenous spaces carrying bi-algebraic structures (such as torii, Abelian varieties and Shimura varieties), Klingler and Lerer recently showed that any bi-algebraic curve in a stratum of the moduli space of Abelian differentials is linear provided that the so-called condition $(\star )$ is fulfilled.In this note, we construct a non-linear bi-algebraic curve, resp. surface, of Abelian differentials of genus $7$, resp. $10$.…”
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708
The platform of spoof videos: The case of Tudou.com
Published 2012-07-01“…Particular reference is made to three “star users”, Jiaoshou, Hu Ge and Corndog, who gained fame for themselves via the popularity of their spoof videos on this platform.…”
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709
Illicium floridanum Florida Anise Tree, Florida Anise
Published 2007-05-01“…It describes the plant’s physical characteristics, including its olive green leaves, reddish-purple flowers, and star-shaped seed pods. The document outlines the plant’s growth habits, preferred growing conditions, and uses in landscaping. …”
Get full text
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710
Rotations in the Space of Split Octonions
Published 2009-01-01“…The new representation of products of the basis units of split octonionic having David's star shape (instead of the Fano triangle) is presented. …”
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711
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712
Correction: Trust in AI: progress, challenges, and future directions
Published 2025-01-01Get full text
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713
Dark Galactic Subhalos and the Gaia Snail
Published 2025-01-01“…We also develop a phenomenological treatment for the diffusion of phase-space spirals caused by gravitational scattering between stars and giant molecular clouds, a process that erases the kinematic signatures of old ( t ≳ 0.6 Gyr) events. …”
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714
Nebular and Nonthermal Radio Emissions for Young Stellar Populations with PARSEC v1.2s
Published 2025-01-01“…In a forthcoming paper, we will use our new SSP libraries as input to the state-of-the-art radiative transfer model GRA phites and SIL icates to test the overall performance of these SSPs in reproducing the observed spectral energy distribution of young star-forming galaxies.…”
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715
MINDS. JWST-MIRI Observations of a Spatially Resolved Atomic Jet and Polychromatic Molecular Wind toward SY Cha
Published 2025-01-01“…The removal of angular momentum from protostellar systems drives accretion onto the central star and may drive the dispersal of the protoplanetary disk. …”
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716
Implication of Galaxy-scale Negative Feedback by One of the Most Powerful Multiphase Outflows in a Hyperluminous Infrared Galaxy at Intermediate Redshift
Published 2025-01-01“…Powerful galactic outflows driven by active galactic nuclei (AGNs) are commonly considered as one of the main mechanisms to regulate star formation in massive galaxies. Ultra- and hyperluminous IR galaxies (U/HyLIRGs) are thought to represent a transition phase of galaxies from a rapidly growing period to a quiescent status as gas is swept out by outflows, providing a laboratory in which to investigate outflows and their feedback effects on hosts. …”
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717
The first photometric investigation of two short-period Algol-type eclipsing binaries: IW UMa and V367 Gem
Published 2025-01-01“…The stellar atmospheric parameters of the primary stars were derived through spectral analysis. Ground-based and TESS-based light curves were analyzed.MethodsULySS software was employed to obtain atmospheric parameters by fitting full spectra with model spectra. …”
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718
The James Webb Space Telescope Absolute Flux Calibration. III. Mid-infrared Instrument Medium Resolution Integral Field Unit Spectrometer
Published 2025-01-01“…Pixel flat fields are constructed from observations of the infrared-bright planetary nebula NGC 7027, and photometric aperture corrections from a combination of theoretical models and observations of bright standard stars. We tie the 5–18 μ m flux calibration to high signal-to-noise ratio (S/N; ∼600–1000) observations of the O9 V star 10 Lacertae, scaled to the average calibration factor of nine other spectrophotometric standards. …”
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719
Exploring the Evolution of a Dwarf Spheroidal Galaxy with SPH Simulations. II. AGN Feedback
Published 2025-01-01“…While AGN feedback is generally negative on star formation, instances of positive feedback were also identified. …”
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720
Insights into the Properties of Type Ibn/Icn Supernovae and Their Progenitor Channels through X-Ray Emission
Published 2025-01-01“…Type Ibn/Icn supernovae (SNe Ibn/Icn), which are characterized by narrow helium or carbon lines that originated in hydrogen-poor dense circumstellar medium (CSM), provide new insights into the final evolution of massive stars. While SNe Ibn/Icn are expected to emit strong X-rays through the strong supernova (SN)-CSM interaction, the X-ray emission modeling effort has been limited so far. …”
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