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The Extended CO(3 - 2) Emission in the Protogalaxy IRAS F10214+4724

Published online by Cambridge University Press:  12 April 2016

Robert L. Brown
Robert L. Brown*
Affiliation:
National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903-2475

Abstract

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Preliminary observations of the z = 2.286 protogalaxy in the redshifted J = 3 − 2 transition of CO made with the Owens Valley Radio Observatory array suggest that the CO emission is spatially extended. This is particularly evident in the narrow band spectral channels. There are indications of CO emission regions in the field of IRAS F10214+4724 that are not related to the IRAS galaxy.

Type
3. Astronomical Results and Prospects
Information
International Astronomical Union Colloquium , Volume 140: Astronomy with Millimeter and Submillimeter Wave Interferometry , 1994 , pp. 332 - 335
Copyright
Copyright © Astronomical Society of the Pacific 1994

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