Results 211 to 220 of about 30,280 (240)

Ultraluminous Infrared Galaxies at 1.5

2007
We present measurements of the spatial clustering of ultraluminous infrared galaxies in two redshift intervals, 1.51.
Farrah, D., Lonsdale, C. J., Borys, C., Fang, F., Waddington, I., Oliver, S., Rowan-Robinson, M., Babbedge, T., Shupe, D., Polletta, M., Smith, H. E., Surace, J.   +11 more
openaire   +1 more source

Ultraluminous Infrared Galaxies: Far-Infrared Highlights

Astrophysics and Space Science, 1999
We discuss two significant recent developments in the far-IRwith relevance to the study of Ultraluminous Infrared Galaxies(ULIRGs). The first of these is the discovery of an isotropiccosmological infrared background radiation (CIB). This has beendetected in observations by two different instruments (FIRAS (Puget etal. 1996, Hauser et al.
openaire   +1 more source

Near-Infrared Spectroscopy of Ultraluminous Infrared Galaxies

1994
We report K band spectra of fourteen ultraluminous (LIR ≥ 1012L⊙) galaxies from the IRAS Extended Bright Galaxy Sample (EBGS) and ten less luminous EBGS galaxies. For the lower luminosity systems, good correlations are found between the H2 v=1-0S(1) and far-infrared (FIR) fluxes, and Brγ and FIR fluxes.
J. D. Goldader, R. D. Joseph, D. B. Sanders, R. Doyon   +3 more
openaire   +1 more source

Molecular Gas in Ultraluminous Infrared Galaxies

1997
The discovery of CO emission (Wilson, Jefferts & Penzias 1970) 25 years ago opened a major new astronomical window which has led to important advances in many areas of Galactic and extragalactic astronomy. The strength and ubiquity of the CO lines, CO isotopic lines, and other millimeter transitions have provided extraordinary diagnostics for studying ...
openaire   +1 more source

Ejection from Ultraluminous Infrared Galaxies

2000
Active galaxies, particularly Seyferts, have been shown to eject material in various forms including quasars with high intrinsic redshifts. A class of active galaxy which has so far not been analyzed from this standpoint is the so called Ultra Luminous Infrared Galaxies (ULRIG’s).
openaire   +1 more source

Near-Infrared Imaging of Ultraluminous IRAS Galaxies

1994
IRAS discovered a class of objects which emit most of their radiation at infrared wavelengths and which possess bolometric luminosities comparable to those of classical quasars. Due to their extreme power, and the fact that (1) they are nearly always in the late stages of a galactic merger, and (2) they have a space density in the local universe ...
Surace, J., Armus, L., Graham, J., Matthews, K., Mazzarella, J., Neugebauer, G., Soifer, B. T.   +6 more
openaire   +2 more sources

InP colloidal quantum dots for visible and near-infrared photonics

Nature Reviews Materials, 2023
Guilherme Almeida
exaly  

Second near-infrared photothermal materials for combinational nanotheranostics

Chemical Society Reviews, 2021
Cheng Xu, Kanyi Pu
exaly  

Power of Infrared and Raman Spectroscopies to Characterize Metal-Organic Frameworks and Investigate Their Interaction with Guest Molecules

Chemical Reviews, 2021
Konstantin I Hadjiivanov, Dimitar A Panayotov, Mihail Mihaylov   +2 more
exaly  

Ultraluminous Infrared Galaxies and Galaxy Formation

Astrophysics and Space Science, 1999
openaire   +1 more source