Results 91 to 100 of about 35,402 (267)
Silicates in Ultraluminous Infrared Galaxies
We analyze the mid-infrared (MIR) spectra of ultraluminous infrared galaxies (ULIRGs) observed with the Spitzer Space Telescope's Infrared Spectrograph. Dust emission dominates the MIR spectra of ULIRGs, and the reprocessed radiation that emerges is independent of the underlying heating spectrum.
Sirocky, M. M.+4 more
openaire +6 more sources
Near‐Infrared and Star‐forming Properties of Local Luminous Infrared Galaxies [PDF]
We use HST NICMOS continuum and Pa-alpha observations to study the near-infrared and star-formation properties of a representative sample of 30 local (d ~ 35-75Mpc) luminous infrared galaxies (LIRGs, infrared 8-1000um luminosities of L_IR=11-11.9[Lsun]).
Alonso Herrero, Almudena+5 more
openaire +6 more sources
Observations of young star clusters in a variety of galaxies have been used to constrain basic properties related to star formation, such as the fraction of stars found in clusters (Γ) and the shape of the cluster mass function (CMF).
Miranda Caputo+5 more
doaj +1 more source
UEG Week 2022 Moderated Posters
United European Gastroenterology Journal, Volume 10, Issue S8, Page 185-472, October 2022.
wiley +1 more source
Neutral Gas Outflows and Inflows in Infrared-Faint Seyfert Galaxies
Previous studies of the Na I D interstellar absorption line doublet have shown that galactic winds occur in most galaxies with high infrared luminosities.
Cooper+54 more
core +1 more source
Pairing statistics for infrared-luminous galaxies
A knowledge of the pairing fraction of IR-selected galaxies is important in understanding the role of interactions in star formation and nuclear activity. It is clear that interactions are extremely common among the most IR-luminous systems, but results have been inconsistent for less luminous systems; this may result from using peculiar morphology as ...
J. F. Gallimore, William C. Keel
openaire +2 more sources
A Complete 16 μm Selected Galaxy Sample at z ∼ 1. II. Morphological Analysis
We present a morphological analysis of the 16 μ m flux-density-limited galaxy sample at 0.8 < z < 1.3 from Huang et al. (2021). At the targeted redshift, the 16 μ m emission corresponds to the polycyclic aromatic hydrocarbon feature from intense star ...
Piaoran Liang+4 more
doaj +1 more source
GOALS-JWST: Small Neutral Grains and Enhanced 3.3 μm PAH Emission in the Seyfert Galaxy NGC 7469
We present James Webb Space Telescope (JWST) Near Infrared Spectrograph (NIRSpec) integral field spectroscopy of the nearby luminous infrared galaxy NGC 7469.
Thomas S.-Y. Lai+39 more
doaj +1 more source
Probing Cool and Warm Infrared Galaxies using Photometric and Structural Measures [PDF]
We have analyzed a sample of nearby cool and warm infrared (IR) galaxies using photometric and structural parameters. The set of measures include far-infrared color ($C = \log_{10}[S_{60\mu m}/S_{100\mu m}]$), total IR luminosity ($L_{TIR}$), radio ...
Alton P. B.+13 more
core +2 more sources
Characterising Nearby Luminous Infrared Galaxies
Luminous InfraRed Galaxies (LIRGs) in the local universe are known to be highly interacting galaxies with strong star-formation in obscured environments. LIRGs have diversity in terms of morphology and mode and location of SF, while their even more energetic counterparts, the Ultra-Luminous IR galaxies, ULIRGs, (LIR ≥ 10^12 Lsol ) are normally ...
Petri Väisänen+2 more
openaire +2 more sources