Results 71 to 80 of about 629 (178)

Possibility of Using 3.3 μm Polycyclic Aromatic Hydrocarbon Luminosity as a Molecular Gas Mass Estimator

open access: yesThe Astrophysical Journal
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

Starbursts in Ultraluminous Infrared Galaxies — Fueling and Properties [PDF]

open access: yes, 2001
6 pages, 3 embedded ps figures; uses svmult.cls and physprbb.sty (included); to appear in "Starburst galaxies - near and far", proceedings of the Ringberg workshop, eds. D. Lutz and L.J. Tacconi (to be published by Springer)
openaire   +2 more sources

Extragalactic Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory. [PDF]

open access: yesSpace Sci Rev, 2023
Aalto S   +7 more
europepmc   +1 more source

Ultraviolet-bright, High-Redshift Ultraluminous Infrared Galaxies

open access: yesThe Astrophysical Journal, 2006
We present Spitzer Space Telescope observations of the z = 2.38 Lyα emitter overdensity associated with galaxy cluster J2143-4423, the largest known structure (110 Mpc) above z = 2. We imaged 22 of the 37 known Lyα emitters within the filament-like structure, using the MIPS 24 μm band.
Colbert, James W   +5 more
openaire   +2 more sources

Polarized thermal emission from dust in a galaxy at redshift 2.6. [PDF]

open access: yesNature, 2023
Geach JE   +7 more
europepmc   +1 more source

Graph Theoretical Analysis of local ultraluminous infrared galaxies and quasars [PDF]

open access: green, 2023
Orestis Pavlou   +5 more
openalex   +1 more source

Ionized Carbon in Galaxies: The [C ii] 158 μm Line as a Total Molecular Gas Mass Tracer Revisited

open access: yesThe Astrophysical Journal
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

Electromagnetic counterparts to massive black-hole mergers. [PDF]

open access: yesLiving Rev Relativ, 2022
Bogdanović T, Miller MC, Blecha L.
europepmc   +1 more source

Erratum: “VLA H53α Radio Recombination Line Observations of the Ultraluminous Infrared Galaxy Arp 220” (ApJ, 633, 198 [2005]) [PDF]

open access: bronze, 2007
C. A. Rodriguez‐Rico   +5 more
openalex   +1 more source

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