Results 1 to 10 of about 3,100 (226)
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The star formation history of luminous infrared galaxies
Astronomy and Astrophysics, 2006D Marcillac +2 more
exaly
An XMM-Newtonstudy of hyper-luminous infrared galaxies
Astronomy and Astrophysics, 2007A Ruiz, F J Carrera, F Panessa
exaly
HST/WFPC2 morphologies and color maps of distant luminous infrared galaxies
Astronomy and Astrophysics, 2004Xianzhong 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, 2003M Contini, Contini Thierry
exaly
HCN Survey of Normal Spiral, Infraredâluminous, and Ultraluminous Galaxies
Astrophysical Journal, Supplement Series, 2004Yu Gao, Philip M Solomon
exaly
PMAS optical integral field spectroscopy of luminous infrared galaxies
Astronomy and Astrophysics, 2009A Alonso-Herrero +2 more
exaly
The Role of AGN in Luminous Infrared Galaxies from the Multiwavelength Perspective
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]
( 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]
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]
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

