Results 71 to 80 of about 5,290 (158)

Sub-arcsecond CO(1-0) and CO(2-1) observations of the ultraluminous infrared galaxy IRAS 10190+1322

, 2007
We present the results of high resolution mapping of the CO(1-0) and CO(2-1) emission of the ultraluminous infrared galaxy (ULIRG) IRAS 10190+1322, with the IRAM interferometer, down to an angular resolution of ~0.3 arcsec. This object is composed of two
Braine, Bushouse, Crawford, Dasyra, Downes, Evans, Farrah, Imanishi, J. Graciá-Carpio, Kim, L. Colina, Lo, Murphy, Murphy, Nagar, P. Planesas, Rupke, Sakamoto, Sanders, Solomon, Spergel, Veilleux, White   +22 more
core   +1 more source

Ultraluminous Infrared Galaxies: Mergers of Sub‐L* Galaxies? [PDF]

The Astrophysical Journal, 2001
A sample of 27 low-redshift, mostly cool, ultraluminous infrared galaxies (ULIRGs) has been imaged at 1.6 μm with the Hubble Space Telescope (HST) Near-Infrared Camera and Multi-Object Spectrometer (NICMOS). The majority (67%) of the sample's galaxies are multiple-nucleus galaxies with projected separations of up to 17 kpc, and the rest of the sample ...
Michael Rowan-Robinson, Kirk D. Borne, Andy Lawrence, A. C. Baker, Seb Oliver, Luis Colina, David L. Clements, Ray A. Lucas, Howard Bushouse   +8 more
openaire   +2 more sources

Optical and Near-Infrared Imaging of the IRAS 1-Jy Sample of Ultraluminous Infrared Galaxies: II. The Analysis

, 2002
The present paper discusses the results from an analysis of the images presented in Paper I (astro-ph/0207373) supplemented with new spectroscopic data obtained at Keck.
Arribas S., Bender R., Clements D. L., D. B. Sanders, D.‐C. Kim, Glazebrook K., Jedrzejewski R., Kawara K., Lawrence A., Leech K. J., Lilly S. J., Matsuhara H., Melnick J., Mobasher B., Puget J. L., S. Veilleux, Sanders D. B., Taylor G. L., Zheng Z., Zou Z., Zucca E.   +20 more
core   +1 more source

Building on the Archives: Connecting the CN/CO Intensity Ratio with Global Galaxy Properties in Nearby U/LIRGs

The Astrophysical Journal
We use the CN/CO intensity ratio to obtain the dense gas fraction, f _dense , for a sample of 16 ultraluminous and luminous infrared (IR) galaxies and compare f _dense with a suite of global galaxy properties.
Blake Ledger, Christine D. Wilson, Osvald Klimi, Núria Torres-Albà, Toshiki Saito   +4 more
doaj   +1 more source

APM 08279+5255: an ultraluminous BAL quasar at a redshift z=3.87

, 1998
We report on the discovery of a highly luminous, broad absorption line quasar at a redshift of $z=3.87$ which is positionally coincident, within one arcsecond, with the IRAS FSC source F08279+5255.
Edward J. Totten, Geraint F. Lewis, Guilloteau S., Hawkins M. R. S., Hook I. M., Kayser R., Michael J. Irwin, Oliver S. J., Prestage R., Rodrigo A. Ibata, Rowan-Robinson M., Sopp H. M., Williams L. L. R., Yee H. K. C.   +13 more
core   +1 more source

A Complete 16 μm Selected Galaxy Sample at z ∼ 1. II. Morphological Analysis

The Astrophysical Journal
We present a morphological analysis of the 16 μ m flux-density-limited galaxy sample at 0.8 < z < 1.3 from Huang et al. (2021). At the targeted redshift, the 16 μ m emission corresponds to the polycyclic aromatic hydrocarbon feature from intense star ...
Piaoran Liang, Y. Sophia Dai, Jia-Sheng Huang, Cheng Cheng, Yaru Shi   +4 more
doaj   +1 more source

Star-Forming AGN Host Galaxies

, 2001
The symbiosis of nuclear activity and star-formation in galaxies, as manifested in their spectral energy distributions (SEDs) is reviewed. Attention is drawn to an Hertzsprung-Russell diagram-equivalent for such objects, as well as to the importance of ...
Bregman, Brown, Canalizo, Canalizo, Clements, Colina, Condon, Condon, De Grijp, Edelson, Giuricin, Golombek, Haas, Haas, Heckman, Heckman, Hes, Hoekstra, Impey, Kewley, Kirhakos, Klaas, Lutz, Lutz, Lutz, Madau, Mazzarella, Miley, Neugebauer, Neugebauer, Peter Barthel, Polletta, Pérez Garcı́a, Rodrı́guez Espinosa, Rodrı́guez Espinosa, Rowan-Robinson, Rush, Sanders, Sanders, Schinnerer, Schmidt, Shaver, Sopp, Spinoglio, Spoon, Taylor, Van Bemmel, Van Bemmel, Willott, Wink   +49 more
core   +3 more sources

Sensitive Radio Observations of High Redshift Dusty QSOs [PDF]

, 1999
We present sensitive radio continuum imaging at 1.4 GHz and 4.9 GHz of seven high redshift QSOs selected for having a 240 GHz continuum detection, which is thought to be thermal dust emission.
Benford D. J., Benford D. J., C. L. Carilli, Cimatti A., Downes D., Guilloteau S., Guilloteau S., Hughes D. H., Isaak K. G., Ivison R. J., K. Kohno, K. Ohta, Lawrence A., M. S. Yun, McMahon R. G., Omont A., R. Kawabe, Y. Tutui   +17 more
core   +2 more sources

JWST Discovery of a Very Fast Biconical Outflow of Warm Molecular Gas in the Nearby Ultraluminous Infrared Galaxy F08572+3915 NW

The Astrophysical Journal
We present new James Webb Space Telescope (JWST) Mid-Infrared Instrument Medium-Resolution Spectrometer observations of the nearby ultraluminous infrared galaxy (ULIRG) F08572+3915 NW. These integral field spectroscopic (IFS) data reveal a kpc-scale warm-
Kylie Yui Dan, Jerome Seebeck, Sylvain Veilleux, David Rupke, Eduardo Gonzalez-Alfonso, Ismael Garcia-Bernete, Weizhe Liu, Dieter Lutz, Marcio Melendez, Miguel Pereira Santaella, Eckhard Sturm, Francesco Tombesi   +11 more
doaj   +1 more source

Extinction law in ultraluminous infrared galaxies at z∼ 1 [PDF]

Monthly Notices of the Royal Astronomical Society, 2011
We analyze the multi-wavelength photometric and spectroscopic data of 12 ultraluminous infrared galaxies (ULIRGs) at z ~ 1 and compare them with models of stars and dust in order to study the extinction law and star formation in young infrared (IR) galaxies.
Shimizu, T., Kawara, K., Sameshima, H., Ienaka, N., Nozawa, T., Kozasa, T.   +5 more
openaire   +5 more sources