High resolution spectral imaging of CO(7-6), [CI](2-1), and continuum of three high-z lensed dusty star-forming galaxies using ALMA

High-redshift dusty star-forming galaxies with very high star formation rates (500-3000 M-circle dot yr(-1)) are key to understanding the formation of the most extreme galaxies in the early Universe. Characterising the gas reservoir of these systems can reveal the driving factor behind the high star...

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Bibliographic Details
Published in:Astronomy & Astrophysics
Main Authors: Gururajan, G., Bethermin, M., Theule, P., Spilker, J. S., Aravena, M., Archipley, M. A., Chapman, S. C., De Breuck, C., Gonzalez, A., Hayward, C. C., Hezaveh, Y., Hill, R., Jarugula, S., Litke, K. C., Malkan, M., Marrone, D. P., Narayanan, D., Phadke, K. A., Reuter, C., Vieira, J. D., Vizgan, D., Weiss, A.
Format: Article in Journal/Newspaper
Language:English
Published: 2022
Subjects:
galaxies
high-redshift
evolution
ISM
kinematics and dynamics
star formation
submillimeter
DEEP FIELD SOUTH
UBIQUITOUS MOLECULAR OUTFLOWS
SIMILAR-TO 4
ATOMIC CARBON
SUBMILLIMETER GALAXIES
INTERSTELLAR-MEDIUM
STARBURST GALAXIES
GAS FRACTIONS
CO
Milky Way
South Pole
South pole
Online Access:https://curis.ku.dk/portal/da/publications/high-resolution-spectral-imaging-of-co76-ci21-and-continuum-of-three-highz-lensed-dusty-starforming-galaxies-using-alma(2063bca6-c80c-4837-9e91-8ea9bf143486).html
https://doi.org/10.1051/0004-6361/202142172
https://curis.ku.dk/ws/files/319527043/aa42172_21.pdf

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