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- W1501431055 abstract "Our knowledge of the process by which cold gas in the early universe accumulates and forms stars is limited by our inability to image the gas. The next generation of millimeter and submillimeter wavelength arrays will allow us to explore the gas content of forming galaxies at the same resolution at which HST and the new 8 m class optical/IR telescopes will reveal early generations of stars. The dust that obscures our view of the early universe at optical wavelengths becomes an asset at millimeter/submillimeter wavelengths where the thermal dust emission can be imaged. With the new millimeter arrays astronomers will: (1) image the mass segregation and kinematics of hierarchical galaxy formation; (2) have the ability to detect thermal dust continuum emission from more than 15 million galaxies with an observation time of less than a minute per galaxy (indeed, such cosmological IR-luminous galaxies will be a source of confusion to every continuum observation); and (3) detect atomic and molecular spectral line emission from normal galaxies such as the Milky Way at redshifts greater than one." @default.
- W1501431055 created "2016-06-24" @default.
- W1501431055 creator A5061305604 @default.
- W1501431055 date "1996-01-01" @default.
- W1501431055 modified "2023-09-23" @default.
- W1501431055 title "Studies of Cold Gas in the Early Universe with Large Millimeter Arrays" @default.
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- W1501431055 doi "https://doi.org/10.1007/978-94-009-1726-2_50" @default.
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