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 …
A survey of high-z galaxies: serra simulations
We introduce serra, a suite of zoom-in high-resolution (, at z= 7.7) cosmological simulations
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …
Mapping Obscuration to Reionization with ALMA (MORA): 2 mm Efficiently Selects the Highest-redshift Obscured Galaxies
CM Casey, JA Zavala, SM Manning… - The Astrophysical …, 2021 - iopscience.iop.org
We present the characteristics of 2 mm selected sources from the largest Atacama Large
Millimeter/submillimeter Array (ALMA) blank-field contiguous survey conducted to date, the …
Millimeter/submillimeter Array (ALMA) blank-field contiguous survey conducted to date, the …
MIDIS: Strong (Hβ+[O iii]) and Hα Emitters at Redshift z≃ 7–8 Unveiled with JWST NIRCam and MIRI Imaging in the Hubble eXtreme Deep Field
We make use of JWST medium-band and broadband NIRCam imaging, along with
ultradeep MIRI 5.6 μm imaging, in the Hubble eXtreme Deep Field to identify prominent line …
ultradeep MIRI 5.6 μm imaging, in the Hubble eXtreme Deep Field to identify prominent line …
The ALPINE-ALMA [CII] survey-Obscured star formation rate density and main sequence of star-forming galaxies at z> 4
Y Khusanova, M Bethermin, O Le Fèvre… - Astronomy & …, 2021 - aanda.org
Star formation rate (SFR) measurements at z> 4 have relied mostly on the rest-frame far-
ultraviolet (FUV) observations. The corrections for dust attenuation based on the IRX-β …
ultraviolet (FUV) observations. The corrections for dust attenuation based on the IRX-β …
The nature of high [O iii]88 μ m/[C ii]158 μm galaxies in the epoch of reionization: Low carbon abundance and a top-heavy IMF?
ABSTRACT ALMA observations of z> 6 galaxies have revealed abnormally high [O iii] 88
m/[C ii] 158 m ratios and [C ii] 158 m deficits compared to local galaxies. The origin of this …
m/[C ii] 158 m ratios and [C ii] 158 m deficits compared to local galaxies. The origin of this …
The Galaxy Starburst/Main-sequence Bimodality over Five Decades in Stellar Mass at z≈ 3–6.5
The Galaxy Starburst/Main-sequence Bimodality over Five Decades in Stellar Mass at z ≈ 3–6.5
- IOPscience Skip to content IOP Science home Accessibility Help Search Journals Journals …
- IOPscience Skip to content IOP Science home Accessibility Help Search Journals Journals …
The ALMA REBELS Survey: The Cosmic H i Gas Mass Density in Galaxies at z≈ 7
The neutral atomic gas content of individual galaxies at large cosmological distances has
until recently been difficult to measure due to the weakness of the hyperfine H i 21 cm …
until recently been difficult to measure due to the weakness of the hyperfine H i 21 cm …
Illuminating the dark side of cosmic star formation two billion years after the Big Bang
M Talia, A Cimatti, M Giulietti, G Zamorani… - The Astrophysical …, 2021 - iopscience.iop.org
How and when did galaxies form and assemble their stars and stellar mass? The answer to
these questions, so crucial to astrophysics and cosmology, requires the full reconstruction of …
these questions, so crucial to astrophysics and cosmology, requires the full reconstruction of …
The ALPINE-ALMA [CII] survey-The contribution of major mergers to the galaxy mass assembly at z∼ 5
M Romano, P Cassata, L Morselli, GC Jones… - Astronomy & …, 2021 - aanda.org
Context. Galaxy mergers are thought to be one of the main mechanisms of the mass
assembly of galaxies in the Universe, but there is still little direct observational evidence of …
assembly of galaxies in the Universe, but there is still little direct observational evidence of …