Results 1 to 10 of about 36,576 (272)

Environmental Dependence of Local Luminous Infrared Galaxies [PDF]

Astronomy & Astrophysics, 2010
We study the environmental dependence of local luminous infrared galaxies (LIRGs) and ultraluminous infrared galaxies (ULIRGs) found in the Sloan Digital Sky Survey (SDSS) data.
Abazajian, Allam, Baldwin, Balogh, Bitsakis, Blanton, Blanton, Brinchmann, Bruzual, C. Park, Capak, Cardelli, Carlberg, Chary, Chen, Choi, Colless, Cooper, D. Elbaz, Dasyra, Elbaz, Falco, Farrah, Feruglio, Gallazzi, Genzel, Gilli, Goto, Gómez, H. M. Lee, H. S. Hwang, Hill, Hill, Hopkins, Hwang, Hwang, Hwang, Ideue, J. C. Lee, Jeong, Kauffmann, Kauffmann, Kennicutt, Kennicutt, Kewley, Kewley, Kim, Koulouridis, Le Floc’h, Le Floc’h, Lee, Lewis, Li, Lotz, M. G. Lee, Magnelli, Marcillac, Murakami, Murphy, Neugebauer, Noeske, Noeske, Owers, Park, Park, Park, Park, Park, Patel, Sanders, Shi, Shi, Slinglend, Soifer, Stoughton, Sutherland, Tanaka, Tran, Tremonti, Veilleux, Veilleux, Veilleux, W.-S. Jeong, Wang, Wang, Wang, Wegner, Wegner, York, Yuan, Zauderer   +90 more
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Statistics of associations among IR galaxies [PDF]

In the course of expanding the search of Kleinmann et. al. (1988) for distant, infrared-luminous objects, the authors noticed (as is often remarked) that a large number of infrared-selected galaxies have close neighbors or show merger characteristics (e ...
Gallimore, Jack F., Keel, William C.
core   +1 more source

Luminosities of Barred and Unbarred S0 Galaxies

, 2012
Lenticular galaxies with M_B < -21.5 are almost exclusively unbarred, whereas both barred and unbarred objects occur at fainter luminosity levels. This effect is observed both for objects classified in blue light, and for those that were classified in ...
Buta, de Vaucouleurs, de Vaucouleurs, Hubble, Sales, Sandage, Sandage, Sandage, Sidney van den Bergh, van den Bergh   +9 more
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EXPLAINING THE [C II]157.7 μm DEFICIT IN LUMINOUS INFRARED GALAXIES—FIRST RESULTS FROM AHERSCHEL/PACS STUDY OF THE GOALS SAMPLE [PDF]

, 2013
T. Díaz-Santos, L. Armus, V. Charmandaris, Sabrina Stierwalt, Edward J. Murphy, S. Haan, Hanae Inami, Sangeeta Malhotra, R. Meijerink, G. J. Stacey, Andreea Petric, A. Evans, Sylvain Veilleux, P. van der Werf, S. Lord, N. Lu, Justin Howell, P. N. Appleton, J. M. Mazzarella, J. A. Surace, C. K. Xu, B. Schulz, D. B. Sanders, Carrie Bridge, B. Chan, D. T. Frayer, K. Iwasawa, J. Melbourne, E. Sturm   +28 more
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The essential signature of a massive starburst in a distant galaxy

, 2003
Observations of carbon monoxide (CO) emission in high redshift (z>2) galaxies indicate the presence of large amounts of molecular gas. Many of these galaxies contain an active galactic nucleus (AGN) powered by accretion of gas onto a supermassive black ...
AA Penzias, C Carilli, C. Carilli, D Downes, GL Granato, J-P Kneib, M. Guelin, P. Solomon, P. Vanden Bout, PM Solomon, PM Solomon, PM Solomon, R Barvainis, R Barvainis, R Plume, S Venturini   +15 more
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A CO, HCN and CI line survey of Ultra Luminous Infrared Galaxies [PDF]

, 2006
Panagiotis Papadopoulos
openalex   +1 more source

The Evolution of the Size and Merger Fraction of Submillimeter Galaxies across 1 < z ≲ 6 as Observed by JWST

The Astrophysical Journal
Precise tracking of the growth in galaxy size and the evolution of merger fractions with redshift is vital for understanding the formation history of submillimeter galaxies (SMGs). This study investigates this evolution over a broad redshift range (1 
Jian Ren, F. S. Liu, Nan Li, Pinsong Zhao, Qifan Cui, Qi Song, Yubin Li, Hao Mo, Hassen M. Yesuf, Weichen Wang, Fangxia An, Xian Zhong Zheng   +11 more
doaj   +1 more source

A COMPARISON OF THE MORPHOLOGICAL PROPERTIES BETWEEN LOCAL ANDz∼ 1 INFRARED LUMINOUS GALAXIES: ARE LOCAL AND HIGH-z(U)LIRGS DIFFERENT? [PDF]

, 2014
Chao-Ling Hung, D. B. Sanders, Caitlin M. Casey, Michael Koss, Kirsten L. Larson, Nicholas Lee, Yanxia Li, Kelly E. Lockhart, Hsin-Yi Shih, Joshua E. Barnes, Jeyhan S. Kartaltepe, Howard A. Smith   +11 more
openalex   +1 more source

Possibility of Using 3.3 μm Polycyclic Aromatic Hydrocarbon Luminosity as a Molecular Gas Mass Estimator

The Astrophysical Journal
We present CO(1–0) observations of 50 star-forming galaxies at 0.01 < z < 0.35, for which 3.3 μ m polycyclic aromatic hydrocarbon (PAH) emission flux or its upper limit is available.
Hyunjin Shim, Junhyun Baek, Dohyeong Kim, Minjin Kim, Hyunmi Song, Gu Lim, Jaejun Cho, Hayeong Jeong, Yejin Jeong, Ye-eun Kang, Dongseob Lee, Junyeong Park, Eunsuk Seo, Junho Song, Been Yeo   +14 more
doaj   +1 more source

An infrared survey of brightest cluster galaxies: Paper I

, 2007
We report on an imaging survey with the Spitzer Space Telescope of 62 brightest cluster galaxies with optical line emission. These galaxies are located in the cores of X-ray luminous clusters selected from the ROSAT All-Sky Survey.
Alastair Edge, Alice C. Quillen, Allen S. W., Andy Fabian, Brian R. McNamara, Brinkmann W., Christopher P. O’Dea, Craig L. Sarazin, Edge A. C., Edge A. C., Fabian A. C., George Privon, Helen Russell, Jacob Noel‐Storr, Jaehong Park, Joel N. Bregman, Jones D. H., Megan Donahue, Nicholas Zufelt, Stefi A. Baum   +19 more
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