Planck’s dusty GEMS

Planck’s dusty GEMS

We present an analysis of high-resolution ALMA interferometry of CO(4-3) line emission and dust continuum in the "Ruby" (PLCK_G244.8+54.9), a bright, gravitationally lensed galaxy at z = 3.0 discovered with the Planck all-sky survey. The Ruby is the brightest of Planck's dusty GEMS, a...

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Bibliographic Details
Main Authors: Cañameras, R., Nesvadba, N., Kneissl, R., Frye, B., Gavazzi, R., Koenig, S., Le Floc’h, E., Limousin, M., Oteo, I., Scott, D.
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: EDP SCIENCES S A 2017
Subjects:
galaxies: starburst
galaxies: high-redshift
submillimeter: galaxies
galaxies: evolution
galaxies: star formation
galaxies: ISM
Online Access:http://hdl.handle.net/10150/625826
http://arizona.openrepository.com/arizona/handle/10150/625826

Internet

http://hdl.handle.net/10150/625826
http://arizona.openrepository.com/arizona/handle/10150/625826

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