Resolving the ISM at the peak of cosmic star formation with ALMA: the distribution of CO and dust continuum in z∼ 2.5 submillimeter galaxies
Abstract We use Atacama Large Millimeter Array (ALMA) observations of four submillimeter
galaxies (SMGs) at z∼ 2–3 to investigate the spatially resolved properties of the interstellar …
galaxies (SMGs) at z∼ 2–3 to investigate the spatially resolved properties of the interstellar …
Molecular gas in distant galaxies from ALMA studies
F Combes - The Astronomy and Astrophysics Review, 2018 - Springer
ALMA is now fully operational, and has been observing in early science mode since 2011.
The millimetric (mm) and sub-mm domain is ideal to tackle galaxies at high redshift, since …
The millimetric (mm) and sub-mm domain is ideal to tackle galaxies at high redshift, since …
Evidence of extended cold molecular gas and dust haloes around z~ 2.3 extremely red quasars with ALMA
Large-scale outflows are believed to be an important mechanism in the evolution of
galaxies. We can determine the impact of these outflows by studying either current galaxy …
galaxies. We can determine the impact of these outflows by studying either current galaxy …
Atomic and molecular gas in IllustrisTNG galaxies at low redshift
We have recently developed a post-processing framework to estimate the abundance of
atomic and molecular hydrogen (H i and H2, respectively) in galaxies in large-volume …
atomic and molecular hydrogen (H i and H2, respectively) in galaxies in large-volume …
A spatially resolved study of cold dust, molecular gas, H II regions, and stars in the z= 2.12 submillimeter galaxy ALESS67. 1
We present detailed studies of az= 2.12 submillimeter galaxy, ALESS67. 1, using sub-
arcsecond resolution ALMA, adaptive optics-aided VLT/SINFONI, and Hubble Space …
arcsecond resolution ALMA, adaptive optics-aided VLT/SINFONI, and Hubble Space …
High resolution modelling of [CII],[CI],[OIII], and CO line emission from the interstellar medium and circumgalactic medium of a star-forming galaxy at z∼ 6.5
The circumgalactic medium (CGM) is a crucial component of galaxy evolution, but thus far its
physical properties are highly unconstrained. As of yet, no cosmological simulation has …
physical properties are highly unconstrained. As of yet, no cosmological simulation has …
SUPER-VI. A giant molecular halo around az∼ 2 quasar
C Cicone, V Mainieri, C Circosta, D Kakkad… - Astronomy & …, 2021 - aanda.org
We present the discovery of copious molecular gas in the halo of cid_346, az= 2.2 quasar
studied as part of the SINFONI survey for Unveiling the Physics and Effect of Radiative …
studied as part of the SINFONI survey for Unveiling the Physics and Effect of Radiative …
Megaparsec-scale structure around the protocluster core SPT2349–56 at z = 4.3
We present an extensive ALMA spectroscopic follow-up programme of the structure
SPT2349–56, one of the most actively star-forming protocluster cores known, to identify …
SPT2349–56, one of the most actively star-forming protocluster cores known, to identify …
Giant galaxy growing from recycled gas: ALMA maps the circumgalactic molecular medium of the Spiderweb in [C i]
BHC Emonts, MD Lehnert… - Monthly Notices of …, 2018 - academic.oup.com
The circumgalactic medium (CGM) of the massive Spiderweb Galaxy, a conglomerate of
merging proto-cluster galaxies at z= 2.2, forms an enriched interface where feedback and …
merging proto-cluster galaxies at z= 2.2, forms an enriched interface where feedback and …
CO line emission from galaxies in the Epoch of Reionization
We study the CO line luminosity (L CO), the shape of the CO spectral line energy distribution
(SLED), and the value of the CO-to-H2 conversion factor in galaxies in the Epoch of …
(SLED), and the value of the CO-to-H2 conversion factor in galaxies in the Epoch of …