Photodissociation and X-Ray-Dominated Regions
MG Wolfire, L Vallini, M Chevance - Annual Review of …, 2022 - annualreviews.org
The radiation from stars and active galactic nuclei (AGNs) creates photodissociation regions
(PDRs) and X-ray-dominated regions (XDRs), where the chemistry or heating is dominated …
(PDRs) and X-ray-dominated regions (XDRs), where the chemistry or heating is dominated …
High-redshift star formation in the Atacama large millimetre/submillimetre array era
JA Hodge, E da Cunha - Royal Society Open Science, 2020 - royalsocietypublishing.org
The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …
An ALMA [C II] Survey of 27 Quasars at z> 5.94
R Decarli, F Walter, BP Venemans… - The Astrophysical …, 2018 - iopscience.iop.org
An ALMA [C ii] Survey of 27 Quasars at z > 5.94 - IOPscience Skip to content IOP Science
home Accessibility Help Search Journals Journals list Browse more than 100 science journal …
home Accessibility Help Search Journals Journals list Browse more than 100 science journal …
A dynamically cold disk galaxy in the early Universe
The extreme astrophysical processes and conditions that characterize the early Universe
are expected to result in young galaxies that are dynamically different from those observed …
are expected to result in young galaxies that are dynamically different from those observed …
Tracing the total molecular gas in galaxies:[CII] and the CO-dark gas
Context. Molecular gas is a necessary fuel for star formation. The CO (1− 0) transition is
often used to deduce the total molecular hydrogen but is challenging to detect in low …
often used to deduce the total molecular hydrogen but is challenging to detect in low …
Physical Properties of 15 Quasars at z≳ 6.5
C Mazzucchelli, E Bañados… - The Astrophysical …, 2017 - iopscience.iop.org
Physical Properties of 15 Quasars at z ≳ 6.5 - IOPscience This site uses cookies. By continuing
to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies …
to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies …
The [C ii] emission as a molecular gas mass tracer in galaxies at low and high redshifts
We present ALMA Band 9 observations of the [C ii] 158 m emission for a sample of 10 main-
sequence galaxies at redshift∼ 2, with typical stellar masses (log M⋆/M⊙∼ 10.0–10.9) and …
sequence galaxies at redshift∼ 2, with typical stellar masses (log M⋆/M⊙∼ 10.0–10.9) and …
The alpine–alma [c ii] survey: Multiwavelength ancillary data and basic physical measurements
We present the ancillary data and basic physical measurements for the galaxies in the
ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey—the first large …
ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey—the first large …
Galaxies in the first billion years after the Big Bang
DP Stark - Annual Review of Astronomy and Astrophysics, 2016 - annualreviews.org
In the past five years, deep imaging campaigns conducted with the Hubble Space
Telescope (HST) and ground-based observatories have delivered large samples of galaxies …
Telescope (HST) and ground-based observatories have delivered large samples of galaxies …
The ALPINE-ALMA [C II] survey-Little to no evolution in the [C II]–SFR relation over the last 13 Gyr
The [C II] 158 μm line is one of the strongest IR emission lines, which has been shown to
trace the star formation rate (SFR) of galaxies in the nearby Universe, and up to z∼ 2 …
trace the star formation rate (SFR) of galaxies in the nearby Universe, and up to z∼ 2 …