Results 131 to 140 of about 36,025 (222)

UGC 2369S: A Kiloparsec-scale Triple Merger Candidate Identified in a Nearby Luminous Infrared Galaxy

The Astrophysical Journal
We present high-spatial-resolution (≲1 $\mathop{.}\limits{^{\prime\prime} }$ 0), multiwavelength observations of UGC 2369S, a nearby luminous infrared galaxy showing three distinct cores separated on kiloparsec scales in near-infrared (NIR) imaging with ...
Yuanze Ding, Michael J. Koss, Fiona A. Harrison, Charles C. Steidel, Connor Auge, Jared Gillette, Erica Hammerstein, Ruancun Li, Macon Magno, Ignacio del Moral-Castro, Alessandro Peca, Claudio Ricci, Yiqing Song, Ezequiel Treister, Zhuyun Zhuang   +14 more
doaj   +1 more source

A Spitzer/IRS Study of Local Luminous Infrared Galaxies

, 2010
We present the first results of our program to study a sample of local luminous infrared galaxies (LIRGs, L_IR = 10^11-10^12 L_sun) with the Spitzer infrared spectrograph (IRS). In these proceedings we investigate the behavior of the 9.7 um silicate feature in LIRGs.
Pereira-Santaella, M, Alonso-Herrero, A, Rieke, G, Colina, L   +3 more
openaire   +3 more sources

An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Physical Properties of z = 2–5 Ultra- and Hyperluminous Infrared Galaxies

The Astrophysical Journal
We report the physical properties of the 18 brightest ( S _870 _μ _m = 12.4–19.2 mJy) and not strongly lensed 870 μ m–selected dusty star-forming galaxies (DSFGs), also known as submillimeter galaxies (SMGs), in the COSMOS field.
Cheng-Lin Liao, Chian-Chou Chen, Wei-Hao Wang, Ian Smail, Y. Ao, S. C. Chapman, U. Dudzevičiūtė, M. Frias Castillo, Minju M. Lee, Stephen Serjeant, A. M. Swinbank, Dominic J. Taylor, Hideki Umehata, Y. Zhao   +13 more
doaj   +1 more source

Pahs, Ionized Gas, and Molecular Hydrogen in Brightest Cluster Galaxies of Cool Core Clusters of Galaxies

, 2011
We present measurements of 5-25 {\mu}m emission features of brightest cluster galaxies (BCGs) with strong optical emission lines in a sample of 9 cool-core clusters of galaxies observed with the Infrared Spectrograph on board the Spitzer Space Telescope.
Aaron Hoffer, Allen, Bevington, Boulanger, Brandl, Brian R. McNamara, Buson, Bîrzan, Calzetti, Cavagnolo, Churazov, Cleary, Cluver, Colless, Dale, Dale, Dale, Donahue, Donahue, Donahue, Donahue, Draine, Egami, Egami, Elston, Farrah, Fazio, Ferland, G. Mark Voit, Geneviève E. de Messières, Genzel, Groves, Hicks, Hicks, Higdon, Ho, Houck, Huber, Hunstead, Hunter, Jaffe, Johnstone, Kaneda, Kennicutt, Laine, Laurent, Leger, Leitherer, Li, Martel, Megan Donahue, O'Dea, O'Dea, O'Dea, Ogle, Ogle, Paul E. J. Nulsen, Peeters, Peterson, Quillen, Rafferty, Rafferty, Rieke, Rigby, Robert W. O’Connell, Rosenberg, Roussel, Sakon, Sloan, Smith, Smith, Snijders, Springel, Thornley, Treyer, Van Kerckhoven, Voit, Voit, Wu   +78 more
core   +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

JADES: Resolving the Stellar Component and Filamentary Overdense Environment of Hubble Space Telescope (HST)-dark Submillimeter Galaxy HDF850.1 at z = 5.18

The Astrophysical Journal
HDF850.1 is the brightest submillimeter galaxy (SMG) in the Hubble Deep Field. It is known as a heavily dust-obscured star-forming galaxy embedded in an overdense environment at z = 5.18.
Fengwu Sun, Jakob M. Helton, Eiichi Egami, Kevin N. Hainline, George H. Rieke, Christopher N. A. Willmer, Daniel J. Eisenstein, Benjamin D. Johnson, Marcia J. Rieke, Brant Robertson, Sandro Tacchella, Stacey Alberts, William M. Baker, Rachana Bhatawdekar, Kristan Boyett, Andrew J. Bunker, Stephane Charlot, Zuyi Chen, Jacopo Chevallard, Emma Curtis-Lake, A. Lola Danhaive, Christa DeCoursey, Zhiyuan Ji, Jianwei Lyu, Roberto Maiolino, Wiphu Rujopakarn, Lester Sandles, Irene Shivaei, Hannah Übler, Chris Willott, Joris Witstok   +30 more
doaj   +1 more source

Shockingly Effective: Cluster Winds as Engines of Feedback in Starburst Galaxy VV 114

The Astrophysical Journal
We present high-resolution Keck Cosmic Web Imager and MUSE integral field unit spectroscopy of VV 114, a local IR-luminous merger undergoing a vigorous starburst and showing evidence of galactic-scale feedback. The high-resolution data allow for spectral
Justin A. Kader, Vivian U, Jeffrey A. Rich, Marina Bianchin, Sean T. Linden, Anne M. Medling, Tanio Diaz-Santos, George C. Privon, Rosalie McGurk, Lee Armus, Loreto Barcos-Mũnoz, Gabriela Canalizo, Vassilis Charmandaris, Aaron S. Evans, Tianmu Gao, Justin Howell, Hanae Inami, Thomas Lai, Kirsten L. Larson, Matthew A. Malkan, María Sánchez-García, Christopher D. Martin, Mateusz Matuszewski, Claire E. Max, Joseph M. Mazzarella, James D. Neill, Nikolaus Z. Prusinski, Raymond Remigio, David Sanders, Yiqing Song, Sabrina Stierwalt, Jason Surace   +31 more
doaj   +1 more source

The mid-infrared emission of local Luminous Infrared Galaxies

, 2006
En este art´ıculo se combinan la sensibilidad de Spitzer y la alta resolucion espacial de T-ReCS en el GeminiSouth para estudiar las propiedades en el infrarrojo (IR) medio de galaxias luminosas infrarrojas (LIRGs) locales (d < 75 Mpc). Las im´agenes de T-ReCS en 8 − 10 µm nos han permitido separar la emision nuclear (formacion estelar y/o AGN) de la ...
openaire   +4 more sources

Extragalactic Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory. [PDF]

Space Sci Rev, 2023
Aalto S, Battersby C, Chin G, Hunt LK, Rigopoulou D, Stark AA, Viti S, Walker CK.   +7 more
europepmc   +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