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Radio Emission from the Andromeda Nebula [PDF]

open access: possibleNature, 1954
OBSERVATIONS have been made at a wave-length of 3.7 m. with interferometers of different resolving powers to determine the distribution of radio brightness across the Andromeda nebula, M31, which has also been investigated at radio wave-lengths by Hanbury Brown and Hazard1.
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August: Planetary and Emission Nebulae

2009
The brilliant teal glow in the center of the Cat’s Eye Nebula impresses visual astronomers with large telescopes. This central bright region, 20 arcsec in diameter, is just a small portion of the much larger (386 arcsec) outer halo that is a 1,000-fold dimmer, and only appears in long-exposure images such as this one.
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Molecular imaging in oncology: Current impact and future directions

Ca-A Cancer Journal for Clinicians, 2022
Martin G Pomper, Steven P Rowe
exaly  

Radiotheranostics in oncology: Making precision medicine possible

Ca-A Cancer Journal for Clinicians, 2023
Eric O Aboagye
exaly  

Metabolomics in cancer research and emerging applications in clinical oncology

Ca-A Cancer Journal for Clinicians, 2021
Daniel R Schmidt   +2 more
exaly  

New Emission Nebulae

Publications of the Astronomical Society of the Pacific, 1946
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New Emission Nebulae (III)

Publications of the Astronomical Society of the Pacific, 1947
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