Results 1 to 10 of about 3,100 (226)
Some of the next articles are maybe not open access.

The star formation history of luminous infrared galaxies

Astronomy and Astrophysics, 2006
D Marcillac   +2 more
exaly  

An XMM-Newtonstudy of hyper-luminous infrared galaxies

Astronomy and Astrophysics, 2007
A Ruiz, F J Carrera, F Panessa
exaly  

HST/WFPC2 morphologies and color maps of distant luminous infrared galaxies

Astronomy and Astrophysics, 2004
Xianzhong Zheng, F Hammer, H Flores
exaly  

Dust-to-gas ratios in the starburst regions of luminous infrared galaxies

Monthly Notices of the Royal Astronomical Society, 2003
M Contini, Contini Thierry
exaly  

HCN Survey of Normal Spiral, Infrared‐luminous, and Ultraluminous Galaxies

Astrophysical Journal, Supplement Series, 2004
Yu Gao, Philip M Solomon
exaly  

PMAS optical integral field spectroscopy of luminous infrared galaxies

Astronomy and Astrophysics, 2009
A Alonso-Herrero   +2 more
exaly  

The Role of AGN in Luminous Infrared Galaxies from the Multiwavelength Perspective

open access: yesUniverse, 2022
Galaxy mergers provide a mechanism for galaxies to effectively funnel gas and materials toward their nuclei and fuel the central starbursts and accretion of supermassive black holes.
Vivian U
doaj   +4 more sources

Morphological classification of local luminous infrared galaxies [PDF]

open access: yesAstronomy and Astrophysics, 2016
( 18 pages, 12 figures, Accepted for publication in A&A )
V Charmandaris   +2 more
exaly   +6 more sources

Environmental dependence of local luminous infrared galaxies [PDF]

open access: yesAstronomy & Astrophysics, 2010
14 pages, 17 figures. To appear in A&A. Paper with high resolution figures is available at http://astro.kias.re.kr/~hshwang/doc/ms_hwang_lirg ...
Hwang, Ho Seong   +6 more
openaire   +3 more sources

Evolution of the ISM in luminous infrared galaxies [PDF]

open access: yesAstronomy and Astrophysics, 2010
Aims. Molecules that trace the high-density regions of the interstellar medium may be used to evaluate the changing physical and chemical environment during the ongoing nuclear activity in (ultra-) luminous infrared galaxies (ULIRGs).Methods. The changing ratios of the HCN (1-0), HNC (1-0), HCO(+) (1-0), CN (1-0) and CN (2-1), and CS (3-2) transitions ...
Willem A Baan, M Spaans
exaly   +3 more sources

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