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Radio Astronomy, ALMA & Interferometric Arrays: Structures & Vocabulary

Radio astronomy measures wavelengths from millimeters to meters that reveal cold molecular gas, synchrotron radiation, pulsars, jets, the CMB, and many sources hidden from optical view. Radio arrays study cold matter, astrochemistry, star formation, black-hole jets, planet-forming disks, and high-redshift galaxies.

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Radio Astronomy, ALMA & Interferometric Arrays: Structures & Vocabulary

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AST-856Radio Astronomy, ALMA & Interferometric Arrays: Foundations→

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AST-858Radio Astronomy, ALMA & Interferometric Arrays: Physical Mechanisms→

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Radio astronomy measures wavelengths from millimeters to meters that reveal cold molecular gas, synchrotron radiation, pulsars, jets, the CMB, and many sources hidden from optical view.

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The relative arrival phase of a wavefront at separated antennas encodes source direction and structure.

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