Results 31 to 40 of about 35,736 (175)

A Spitzer study of interacting luminous and ultra-luminous infrared galaxies [PDF]

open access: yesProceedings of the International Astronomical Union, 2011
AbstractWe conducted a Spitzer Space Telescope survey of 28 Luminous (11 < log (LIR/L⊙) < 12, LIRGs) and Ultra-Luminous Infrared Galaxies (log (LIR/L⊙) > 12, ULIRGs). Many of these galaxies are found in pairs or associations and are powered by either nuclear activity or star-formation (Sanders & Mirabel 1996).
Claus Leitherer, João R.S. Leão
openaire   +3 more sources

NICMOS Observations of Interaction Triggered Star Formation in the Luminous Infrared Galaxy NGC 6090 [PDF]

open access: yes, 1999
High resolution, 1.1, 1.6, and 2.2 micron imaging of the luminous infrared galaxy NGC 6090 obtained with NICMOS of the Hubble Space Telescope are presented.
Dinshaw, N.   +4 more
core   +2 more sources

The Most Luminous Galaxies [PDF]

open access: yes, 2002
Ultraluminous galaxies in the local universe (z$\leq$0.2) emit the bulk of their energy in the mid and far-infrared. The multiwavelength approach to these objects has shown that they are advanced mergers of gas-rich spiral galaxies.
Mirabel, I. Felix
core   +3 more sources

Star-formation histories of local luminous infrared galaxies [PDF]

open access: yesAstronomy & Astrophysics, 2015
We present the analysis of the integrated spectral energy distribution (SED) from the ultraviolet (UV) to the far-infrared and H$ $ of a sample of 29 local systems and individual galaxies with infrared (IR) luminosities between 10^11 Lsun and 10^11.8 Lsun.
Luis Colina   +11 more
openaire   +10 more sources

Mid-Infrared Spectral Diagnostics of Luminous Infrared Galaxies [PDF]

open access: yesAIP Conference Proceedings, 2010
We present a statistical analysis of 248 luminous infrared galaxies (LIRGs) which comprise the Great Observatories All‐sky LIRG Survey (GOALS) observed with the Infrared Spectrograph (IRS) on‐board Spitzer in the rest‐frame wavelength range between 5 and 38 μm.
A. Petric   +2 more
openaire   +4 more sources

The obscured hyper-energetic GRB 120624B hosted by a luminous compact galaxy at z = 2.20 [PDF]

open access: yes, 2013
Gamma-ray bursts are the most luminous explosions that we can witness in the Universe. Studying the most extreme cases of these phenomena allows us to constrain the limits for the progenitor models. In this Letter, we study the prompt emission, afterglow,
Campana, S.   +13 more
core   +3 more sources

Spatially Resolved [FeII] 1.64 \mu m Emission in NGC 5135. Clues for Understanding the Origin of the Hard X-rays in Luminous Infrared Galaxies [PDF]

open access: yes, 2012
Spatially resolved near-IR and X-ray imaging of the central region of the Luminous Infrared Galaxy NGC 5135 is presented. The kinematical signatures of strong outflows are detected in the [FeII]1.64 \mu m emission line in a compact region at 0.9 kpc from
A. Alonso-Herrero   +32 more
core   +3 more sources

Asca Observations of Luminous Infrared Starburst Galaxies [PDF]

open access: yesSymposium - International Astronomical Union, 1999
We present recent results of X-ray observations of two luminous infrared galaxies, NGC3690+IC694 (Arp299) and NGC1614 obtained by the Japanese X-ray astronomical satellite ASCA. Both galaxies have quite high infrared luminosity (> 1011L⊙) and strong evidence of merger.
T. Nakagawa   +3 more
openaire   +2 more sources

Optical Properties of 4248 IRAS Galaxies

open access: yes, 2005
We have investigated optical properties of 4248 infrared galaxies (IRGs) by positionally matching data from the IRAS and the SDSS DR3. Our sample includes 3 hyper luminous infrared galaxies (L >10^13Lsun) and 178 ultra luminous infrared galaxies (10 ...
Abazajian   +84 more
core   +1 more source

AEGIS: Infrared Spectroscopy of An Infrared Luminous Lyman Break Galaxy at z=3.01 [PDF]

open access: yes, 2006
We report the detection of rest--frame 6.2 and 7.7 \micron emission features arising from Polycyclic Aromatic Hydrocarbons (PAH) in the Spitzer/IRS spectrum of an infrared-luminous Lyman break galaxy at z=3.01.
B. McLeod   +19 more
core   +4 more sources

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