ALMA observations of atomic carbon in z ∼ 4 dusty star-forming galaxies

Abstract We present Atacama Large Millimeter Array [C i](1 − 0) (rest frequency 492 GHz) observations for a sample of 13 strongly lensed dusty star-forming galaxies (DSFGs) originally discovered at 1.4 mm in a blank-field survey by the South Pole Telescope (SPT). We compare these new data with avail...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2017-04, Vol.466 (3), p.2825-2841
Hauptverfasser:	Bothwell, M. S., Aguirre, J. E., Aravena, M., Bethermin, M., Bisbas, T. G., Chapman, S. C., De Breuck, C., Gonzalez, A. H., Greve, T. R., Hezaveh, Y., Ma, J., Malkan, M., Marrone, D. P., Murphy, E. J., Spilker, J. S., Strandet, M., Vieira, J. D., Weiß, A.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Carbon Cosmology and Extra-Galactic Astrophysics Density Dust Field strength Galactic Astrophysics Galaxies Photodissociation Radio telescopes Red shift Sciences of the Universe Star & galaxy formation Star formation Starbursts
Online-Zugang:	Volltext bestellen
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Beschreibung
Zusammenfassung:	Abstract We present Atacama Large Millimeter Array [C i](1 − 0) (rest frequency 492 GHz) observations for a sample of 13 strongly lensed dusty star-forming galaxies (DSFGs) originally discovered at 1.4 mm in a blank-field survey by the South Pole Telescope (SPT). We compare these new data with available [C i] observations from the literature, allowing a study of the interstellar medium (ISM) properties of ∼30 extreme DSFGs spanning a redshift range 2
ISSN:	0035-8711 1365-2966
DOI:	10.1093/mnras/stw3270