English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

We report IRAM Plateau de Bure, millimeter interferometry of three z=~2.4 to3.4, SCUBA deep field galaxies. Our CO line observations confirm the rest-frameUV/optical redshifts, thus more than doubling the number of confirmed,published redshifts of the faint submillimeter population and proving theirhigh-z nature. In all three sources our measurements of the intrinsic gas anddynamical mass are large (1e10 to 1e11 Msun). In at least two cases the datashow that the submillimeter sources are part of an interacting system. Togetherwith recent information gathered in the X-ray, optical and radio bands ourobservations support the interpretation that the submm-population consists ofgas rich (gas to dynamical mass ratio ~0.5) and massive, compositestarburst/AGN systems, which are undergoing a major burst of star formation andare evolving into m*-galaxies.Comment: only minor modifications to comply with the ApJL edition rule

Interferometric Observations of Powerful CO Emission from Three Submillimeter Galaxies at z =2.39, 2.51, and 3.35