Results 81 to 90 of about 149 (141)
We present CO(1–0) observations of 50 star-forming galaxies at 0.01 < z < 0.35, for which 3.3 μ m polycyclic aromatic hydrocarbon (PAH) emission flux or its upper limit is available.
Hyunjin Shim +14 more
doaj +1 more source
Optical versus Mid‐infrared Spectroscopic Classification of Ultraluminous Infrared Galaxies
15 pages, 2 tables, and 3 eps figures.
Taniguchi, Yoshiaki +3 more
openaire +2 more sources
Isomer-specific kinetics of the C+ + H2O reaction at the temperature of interstellar clouds. [PDF]
Yang T +7 more
europepmc +1 more source
Ionized Carbon in Galaxies: The [C ii] 158 μm Line as a Total Molecular Gas Mass Tracer Revisited
In this paper, we present a statistical study of the [C ii ] 158 μ m line and the CO(1−0) emission for a sample of ∼200 local and high- z (32 sources with z > 1) galaxies with very different physical conditions.
Yinghe Zhao +3 more
doaj +1 more source
Ultraluminous Infrared Galaxies and the Origin of QSOs
LaTex, 11 pages with 7 embedded postscript figures, Review presented at the Workshop on "QSO Hosts and Their Environments", Granada, Spain, 10-12 January ...
openaire +2 more sources
High-redshift star formation in the Atacama large millimetre/submillimetre array era. [PDF]
Hodge JA, da Cunha E.
europepmc +1 more source
Powerful galactic outflows driven by active galactic nuclei (AGNs) are commonly considered as one of the main mechanisms to regulate star formation in massive galaxies.
Xiaoyang Chen +14 more
doaj +1 more source
Highlights: optical/NIR spectroscopy of ultraluminous infrared galaxies
This paper reviews the results from recent optical and near-infrared spectroscopic studies of ultraluminous infrared galaxies.
openaire +2 more sources
We report Atacama Large Millimeter/submillimeter Array and Atacama Compact Array observations of atomic carbon ([C i ](1–0)) and dust continuum in 10 enormous Ly α nebulae hosting ultraluminous Type-I QSOs at z = 2.2–2.5, as part of the Survey of ...
Jianan Li +15 more
doaj +1 more source
We observed the X-ray-bright ultraluminous infrared galaxy IRAS 05189−2524 with XRISM during its performance verification phase. The unprecedented energy resolution of the onboard X-ray microcalorimeter revealed complex spectral features at ∼7–9 keV ...
Hirofumi Noda +19 more
doaj +1 more source

