Results 221 to 230 of about 3,156,291 (263)
Association between CVAI-defined body composition phenotypes and prediabetes outcomes in Chinese adults undergoing health check-ups: a cross-sectional study. [PDF]
Front NutrLin R, Jiang W, Wang D, Xu L, Du Y.
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Low Phase Angle as a Clinical Marker of Sarcopenia in Older Adults: Exploring the Structure-Quality-Strength-Mobility (SQSM) Framework. [PDF]
J Frailty Sarcopenia FallsRahman SA +8 more
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Solitary Fibrous Tumor of the Greater Omentum with Intratumoral Infarction: A Case Report. [PDF]
Surg Case RepFuno T +7 more
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Sheath-Liquid CE-MS Interface: A Robust Infusion Platform for Native IMS-MS Analysis of Protein Assemblies and Their Conformers. [PDF]
J Mass SpectromPathak K, Brinkman D, Gomes FP.
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A low-mass star with a large-mass planet
Science, 2023A large planet orbiting a very low-mass star challenges theories of planet ...
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Astrophysics and Space Science, 1994
Low mass stars contribute an important fraction to the mass of our Galaxy. Due to the faintness of these stars a direct investigation of their space distribution and kinematics can be carried out only in the immediate solar neighbourhood. This fact emphasizes the importance of the “Third Catalogue of Nearby Stars” (CNS3) as a probe of the stellar ...
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Low mass stars contribute an important fraction to the mass of our Galaxy. Due to the faintness of these stars a direct investigation of their space distribution and kinematics can be carried out only in the immediate solar neighbourhood. This fact emphasizes the importance of the “Third Catalogue of Nearby Stars” (CNS3) as a probe of the stellar ...
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Mass spectrometry at low and high mass
Current Opinion in Chemical Biology, 1997The introduction of novel methods as well as expanding applications to diverse areas highlight truly impressive progress in mass spectrometry. These developments are illustrated here by two seemingly different areas of research: new methods designed for the determination of isotopic enrichment and novel ionization methods; and mass analyzers which have
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Origins of life and evolution of the biosphere, 1997
Recent evidence indicates that most low mass stars in the Galaxy (< 5 M [symbol: see text]) form alongside massive stars in clusters embedded in giant molecular clouds. Once their parental gas is removed, the fate of these clusters is to disperse and blend into the field population of the galactic disk.
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Recent evidence indicates that most low mass stars in the Galaxy (< 5 M [symbol: see text]) form alongside massive stars in clusters embedded in giant molecular clouds. Once their parental gas is removed, the fate of these clusters is to disperse and blend into the field population of the galactic disk.
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Low-mass red giants and masses of NPNs
Astrophysics and Space Science, 1992The evolutionary track of low-mass red giant stars (0.7–0.9M⊙) is computed with the aim to demonstrate the conditions under which low-mass white dwarfs (WDs) can form through the evolution of single stars. Also, the influence of the mixing length to the scale height ratio on the radius of the star is calculated and the coupling between the mixing ...
Amos Harpaz, Giora Shaviv
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