A Vision for the Future of Astrochemistry in the Interstellar Medium by 2050. [PDF]
Fortenberry RC.
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Effects of Seed Processing with Cold Plasma on Growth and Biochemical Traits of Stevia rebaudiana Bertoni Under Different Cultivation Conditions: In Soil Versus Aeroponics. [PDF]
Judickaitė A+10 more
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In situ Fe-doped thin carbon wires via AC high voltage arc discharge. [PDF]
Jankowski K+9 more
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AI-driven high-throughput droplet screening of cell-free gene expression. [PDF]
Zhu J+11 more
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Optical control of 4f orbital state in rare-earth metals. [PDF]
Thielemann-Kühn N+30 more
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Identification of a turnover in the initial mass function of a young stellar cluster down to 0.5 MJ
De Furio M+13 more
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A freely precessing magnetar following an X-ray outburst. [PDF]
Desvignes G+12 more
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A WC/WO star exploding within an expanding carbon–oxygen–neon nebula
Nature, 2021The final fate of massive stars, and the nature of the compact remnants they leave behind (black holes and neutron stars), are open questions in astrophysics. Many massive stars are stripped of their outer hydrogen envelopes as they evolve.
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Diffuse Einstein X-ray emission from the region of RCW 49, a bright southern emission nebula
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