Luminous infrared galaxies or LIRGs are galaxies with luminosities, the measurement of brightness, above 10 11 L☉. They are also referred to as submillimeter galaxies (SMGs) …

2009年8月17日 · We found 62 Type I ULIRGs, and estimated their BH masses and velocity dispersions from their optical spectra. Together with known Type I ULIRGs in the literature, a …

2006年3月1日 · In this review we look at recent progress on understanding the physics and evolution of local ULIRGs, the contribution of high redshift ULIRGs to the cosmic infrared …

亮紅外星系 或LIRGs是亮度量測上，具有紅外 光度 高於10 11 L☉ 的 星系。 通過正常的檢測方法，它們也被稱為次毫米星系 (SMGs)。 在比較光度時，亮紅外星系遠比 星暴星系 、 西佛星系 …

2024年7月8日 · We present a comprehensive study of Ultraluminous Infrared Galaxies (ULIRGs), leveraging data from the IRAS Faint Source Catalogue (FSC) and the spectroscopic catalog in …

Ultraluminous infrared galaxies (ULIRGs) were recognized as an important population in the local universe more than ten years ago after the IRAS mission. Most of their energy output is dust …

We present radio observations of ultraluminous infrared galaxies (ULIRGs) using the Giant Metrewave Radio Telescope (GMRT) and combine them with archival multifrequency …

Ultraluminous infrared galaxies (ULIRGs) are probably the local analogues of a major mode of galaxy formation in the early universe. Here we give a brief progress report on our on-going …

We present the latest results in our efforts to produce a complete, large sample of ultraluminous infrared galaxies (ULIRGs, L 60 >10 L ⊙ for H 0 =100 km s Mpc , q 0=0.5 ) for use in the …

ULIRGs are generally under-luminous in the X-rays compared to classical AGN, requiring sensitive, high energy, observations to detect them. Evidence for very high X-ray obscuring …