Relevant bibliographies by topics / Ultra luminous IR galaxies

Academic literature on the topic 'Ultra luminous IR galaxies'

Author: Grafiati
Published: 10 December 2022
Last updated: 28 January 2023

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Journal articles on the topic "Ultra luminous IR galaxies"

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Tan, Qinghua, Yu Gao, Zhong Wang, and Vivian U. "High resolution SMA imaging of (ultra)-luminous infrared galaxies." Proceedings of the International Astronomical Union 7, S284 (September 2011): 471–74. http://dx.doi.org/10.1017/s1743921312009659.

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AbstractWe present preliminary results on Submillimeter Array (SMA) observations of three Luminous Infrared Galaxies (LIRGs) and one infrared Quasi Stellar Object (IR QSO). The galaxies were observed at sub-kpc spatial resolution in lines of CO and 13CO, as well as in the continuum at 1.3mm. The moment maps show that the molecular gas in these galaxies is distributed in rotating disks with velocity gradients ranging from ~30 to 120 km s−1 kpc−1. Combined with archival CO J=3-2 data, the spatial distributions of the CO J=3-2/J=2-1 ratios shows clear variations across the galaxies. The brightness temperature of the overlap region in VV 114 is found to be lower than that in the nuclear region of VV 114E, suggesting that that the bulk of molecular gas in this region is sub-thermalized.
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Tyson, J. Anthony. "Spectrum and Origin of the Extragalactic Optical Background Radiation." Symposium - International Astronomical Union 139 (1990): 245–55. http://dx.doi.org/10.1017/s0074180900240813.

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Ultra-deep CCD surveys to 29 mag from .32 to .9 μ wavelength reveal an isotropic population of very blue galaxies. There are over 150,000 of these objects per square degree per magnitude. Saturation of their number density at 27 mag indicates that most of the optical light from this population has been detected. The resulting extragalactic background radiation from the UV to the near-IR due to this population of objects is shown. Gravitational lens and Lyman-break observations show that the redshift of galaxies fainter than 24 mag is in the range 1–3. Small-scale dark lane structures may be intergalactic dust clouds or tunnels through the luminous galaxy distribution.
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Hogan, L., D. Rigopoulou, G. E. Magdis, M. Pereira-Santaella, I. García-Bernete, N. Thatte, K. Grisdale, and J.-S. Huang. "Integral field spectroscopy of luminous infrared main-sequence galaxies at cosmic noon." Monthly Notices of the Royal Astronomical Society 503, no. 4 (February 26, 2021): 5329–50. http://dx.doi.org/10.1093/mnras/stab527.

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ABSTRACT We present the results of an integral field spectroscopy survey of a sample of dusty (ultra) luminous infrared galaxies (U/LIRGs) at 2 < z < 2.5 using KMOS on the Very Large Telescope. The sample has been drawn from Herschel deep field surveys and benefits from ancillary multiwavelength data. Our goal is to investigate the physical characteristics, kinematics, and the drivers of star formation in the galaxies whose contribution dominates the peak of the cosmic star formation density. Two-thirds of the sample are main-sequence galaxies in contrast to the starburst nature of local U/LIRGs. Our kinematic study, unique in its focus on z ∼ 2 dusty star-forming galaxies, uses the H α emission line to find that ∼40 per cent appear to be isolated discs based on the ratio of rotational velocity to the velocity dispersion, suggesting steady-state mechanisms are sufficient to power the large star formation rates (SFRs). The ratio of obscured to unobscured star formation indicates the sample of galaxies experiences less dust obscuration compared to intermediate and local counterparts, while also hosting cooler dust than local U/LIRGs. In addition to H α we detect [N ii] 6583 Å in our targets and show the gas-phase metallicities do not exhibit the metal deficiency of local U/LIRGs. These results indicate that, despite their extreme IR luminosity, the underlying mechanisms driving the massive SFRs found at cosmic noon are due to scaled up disc galaxies as opposed to mergers.
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Greve, Thomas R. "Probing star formation relations of mergers and normal galaxies across the CO ladder." Proceedings of the International Astronomical Union 11, S315 (August 2015): 49–52. http://dx.doi.org/10.1017/s1743921316007249.

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AbstractWe examine integrated luminosity relations between the IR continuum and the CO rotational ladder observed for local (ultra) luminous infra-red galaxies ((U)LIRGs, LIR ≥ 1011 M⊙) and normal star forming galaxies in the context of radiation pressure regulated star formation proposed by Andrews & Thompson (2011). This can account for the normalization and linear slopes of the luminosity relations (log LIR = α log L'CO + β) of both low- and high-J CO lines observed for normal galaxies. Super-linear slopes occur for galaxy samples with significantly different dense gas fractions. Local (U)LIRGs are observed to have sub-linear high-J (Jup > 6) slopes or, equivalently, increasing LCOhigh-J/LIR with LIR. In the extreme ISM conditions of local (U)LIRGs, the high-J CO lines no longer trace individual hot spots of star formation (which gave rise to the linear slopes for normal galaxies) but a more widespread warm and dense gas phase mechanically heated by powerful supernovae-driven turbulence and shocks.
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Klaas, U., M. Haas, S. A. H. Müller, R. Chini, B. Schulz, I. Coulson, H. Hippelein, K. Wilke, M. Albrecht, and D. Lemke. "Infrared to millimetre photometry of ultra-luminous IR galaxies : New evidence favouring a 3-stage dust model." Astronomy & Astrophysics 379, no. 3 (December 2001): 823–44. http://dx.doi.org/10.1051/0004-6361:20011377.

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Ricci, C., G. C. Privon, R. W. Pfeifle, L. Armus, K. Iwasawa, N. Torres-Albà, S. Satyapal, et al. "A hard X-ray view of luminous and ultra-luminous infrared galaxies in GOALS – I. AGN obscuration along the merger sequence." Monthly Notices of the Royal Astronomical Society 506, no. 4 (July 19, 2021): 5935–50. http://dx.doi.org/10.1093/mnras/stab2052.

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ABSTRACT The merger of two or more galaxies can enhance the inflow of material from galactic scales into the close environments of active galactic nuclei (AGNs), obscuring and feeding the supermassive black hole (SMBH). Both recent simulations and observations of AGN in mergers have confirmed that mergers are related to strong nuclear obscuration. However, it is still unclear how AGN obscuration evolves in the last phases of the merger process. We study a sample of 60 luminous and ultra-luminous IR galaxies (U/LIRGs) from the GOALS sample observed by NuSTAR. We find that the fraction of AGNs that are Compton thick (CT; $N_{\rm H}\ge 10^{24}\rm \, cm^{-2}$) peaks at $74_{-19}^{+14}{{\ \rm per\ cent}}$ at a late merger stage, prior to coalescence, when the nuclei have projected separations (dsep) of 0.4–6 kpc. A similar peak is also observed in the median NH [$(1.6\pm 0.5)\times 10^{24}\rm \, cm^{-2}$]. The vast majority ($85^{+7}_{-9}{{\ \rm per\ cent}}$) of the AGNs in the final merger stages (dsep ≲ 10 kpc) are heavily obscured ($N_{\rm H}\ge 10^{23}\rm \, cm^{-2}$), and the median NH of the accreting SMBHs in our sample is systematically higher than that of local hard X-ray-selected AGN, regardless of the merger stage. This implies that these objects have very obscured nuclear environments, with the $N_{\rm H}\ge 10^{23}\rm \, cm^{-2}$ gas almost completely covering the AGN in late mergers. CT AGNs tend to have systematically higher absorption-corrected X-ray luminosities than less obscured sources. This could either be due to an evolutionary effect, with more obscured sources accreting more rapidly because they have more gas available in their surroundings, or to a selection bias. The latter scenario would imply that we are still missing a large fraction of heavily obscured, lower luminosity ($L_{2-10}\lesssim 10^{43}\rm \, erg\, s^{-1}$) AGNs in U/LIRGs.
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Richards, A. M. S., R. J. Cohen, G. H. Cole, A. J. Holloway, A. Pedlar, J. L. Collett, J. H. Knapen, et al. "Circumnuclear Dynamics in Mrk 273 and Mrk 231." Symposium - International Astronomical Union 205 (2001): 212–15. http://dx.doi.org/10.1017/s0074180900221001.

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Markarian 273 and Markarian 231 are ultra-luminous IR galaxies which show signs of merger activity. Their radio continuum and spectral line emission has been imaged on scales of tens of parsec using MERLIN. Mrk 273 and Mrk 231 are classed as Seyfert types 2 and 1 respectively. The distribution and velocity gradients shown by OH masers and HI absorption are consistent with material in a rotating disk or ring, with the axis at greater than 45° to the line of sight in Mrk 273, and at less than 45° to the line of sight in Mrk 231. We estimate the amount of mass enclosed and infer its distribution from irregularities in the maser morphologies and comparison with HI and radio continuum data.
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Mickaelian, Areg M., and Gohar S. Harutyunyan. "Study of the Byurakan-IRAS galaxy sample." Proceedings of the International Astronomical Union 8, S292 (August 2012): 159. http://dx.doi.org/10.1017/s1743921313000896.

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AbstractThe Byurakan-IRAS Galaxy (BIG) sample (Mickaelian 1995) is the result of optical identifications of IRAS PSC sources at high-galactic latitudes using the First Byurakan Survey (FBS) low-dispersion spectra (Markarian et al. 1989). Among the 1577 objects 1178 galaxies have been identified. Most are dusty spiral galaxies and there are a number of ULIRGs among these objects. Our spectroscopic observations carried out with three telescopes (Byurakan Astrophysical Observatory 2.6m, Russian Special Astrophysical Observatory 6m and Observatoire de Haute Provence 1.93m) (Mickaelian & Sargsyan 2010) for 172 galaxies, as well as the SDSS DR8 spectra for 83 galaxies make up the list of 255 spectroscopically studied BIG objects. The classification to activity types for narrow-line emission galaxies has been carried out using the diagnostic diagrams by Veilleux & Osterbrock (1987). All possible physical characteristics have been measured and/or calculated, including radial velocities and distances, angular and physical sizes, absolute magnitudes and luminosities (both optical and IR). IR luminosities and star-formation rates have been calculated from the IR fluxes (Duc et al. 1997).Among the 172 observed galaxies, 102 starburst (HII) ones, 29 AGN (Sy or LINER), and 19 galaxies with composite spectrum have been revealed; spectra of 12 galaxies show emission features but without a possibility for more accurate classification, 9 galaxies are presented as galaxies where the star formation rate does not exceed normal one, and 1 galaxy is an absorption galaxy. Among the 83 objects having SDSS spectra, there are 55 HIIs, 8 Seyferts, 2 LINERs, 4 other AGN (without accurate classification), 6 composite spectrum objects and 8 other emission-line galaxies. In our spectroscopic sample we have 43 (17%) AGN, 25 (10%) composite spectrum objects, 157 (62%) starbursts, 29 emission-line galaxies without a definite type, and 1 absorption-line galaxy. There are 3 Ultra-Luminous InfraRed Galaxies (ULIRG).Various multiwavelength (MW) data have been retrieved for the full sample of 1178 objects from recent catalogs from X-ray to radio (ROSAT, GALEX, APM, MAPS, USNO, GSC, SDSS, 2MASS, WISE, IRAS, AKARI, NVSS, FIRST, etc.) to make a complete study of these galaxies possible. MW SEDs have been built, which have been matched to their optical classifications. Star-formation rates have been calculated to compare to their other physical characteristics, such as morphology, activity types, UV, optical, IR and radio luminosities, etc.
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Ramón-Pérez, Marina, Ángel Bongiovanni, Ana María Pérez García, Jordi Cepa, Jakub Nadolny, Irene Pintos-Castro, Maritza A. Lara-López, et al. "The OTELO survey." Astronomy & Astrophysics 631 (October 14, 2019): A11. http://dx.doi.org/10.1051/0004-6361/201833296.

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Aims. We take advantage of the capabilities of the OSIRIS Tunable Emission Line Object (OTELO) survey to select and study the AGN population in the field. In particular, we aim to perform an analysis of the properties of these objects, including their demography, morphology, and IR luminosity. Focusing on the population of Hα emitters at z ∼ 0.4, we also aim to study the environments of AGN and non-AGN galaxies at that redshift. methods. We make use of the multiwavelength catalogue of objects in the field compiled by the OTELO survey, unique in terms of minimum flux and equivalent width. We also take advantage of the pseudo-spectra built for each source, which allow the identification of emission lines and the discrimination of different types of objects. Results. We obtained a sample of 72 AGNs in the field of OTELO, selected with four different methods in the optical, X-rays, and mid-infrared bands. We find that using X-rays is the most efficient way to select AGNs. An analysis was performed on the AGN population of OTELO in order to characterise its members. At z ∼ 0.4, we find that up to 26% of our Hα emitters are AGNs. At that redshift, AGNs are found in identical environments to non-AGNs, although they represent the most clustered group when compared to passive and star-forming galaxies. The majority of our AGNs at any redshift were classified as late-type galaxies, including a 16% proportion of irregulars. Another 16% of AGNs show signs of interactions or mergers. Regarding the infrared luminosity, we are able to recover all the luminous infrared galaxies (LIRGs) in the field of OTELO up to z ∼ 1.6. We find that the proportion of LIRGs and ultra-luminous infraed galaxies (ULIRGs) is higher among the AGN population, and that ULIRGs show a higher fraction of AGNs than LIRGs.
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Penney, J. I., A. W. Blain, R. J. Assef, T. Diaz-Santos, J. González-López, C.-W. Tsai, M. Aravena, et al. "Cold molecular gas and free–free emission from hot, dust-obscured galaxies at z ∼ 3." Monthly Notices of the Royal Astronomical Society 496, no. 2 (June 6, 2020): 1565–78. http://dx.doi.org/10.1093/mnras/staa1582.

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ABSTRACT We report on observations of redshifted CO(1–0) line emission and observed-frame $\rm \sim 30\,$GHz radio continuum emission from five ultra-luminous, mid-IR selected hot, Dust-Obscured Galaxies (Hot DOGs) at $z\rm \gtrsim 3$ using the Karl G. Jansky Very Large Array. We detect CO(1–0) line emission in all five Hot DOGs, with one of them at high signal-to-noise ratio. We analyse FIR-radio spectral energy distributions, including dust, free–free, and synchrotron emission for the galaxies. We find that most of the $\rm 115\,$ GHz rest-frame continuum is mostly due to synchrotron or free–free emission, with only a potentially small contribution from thermal emission. We see a deficit in the rest-frame $\rm 115\,$ GHz continuum emission compared to dusty star-forming galaxies and sub-millimetre galaxies (SMGs) at high redshift, suggesting that Hot DOGs do not have similar cold gas reserves compared with star-forming galaxies. One target, W2305−0039, is detected in the FIRST $\rm 1.4\, GHz$ survey, and is likely to possess compact radio jets. We compare to the FIR–radio correlation, and find that at least half of the Hot DOGs in our sample are radio-quiet with respect to normal galaxies. These findings suggest that Hot DOGs have comparably less cold molecular gas than star-forming galaxies at lower, $z\rm \sim 2$ redshifts, and are dominated by powerful, yet radio-quiet AGN.
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Dissertations / Theses on the topic "Ultra luminous IR galaxies"

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Sopp, Hazel Marina. "The physics of Ultra-Luminous Infrared Galaxies." Thesis, University of Cambridge, 1991. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.387014.

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Müller, Sven Archibald Hubertus. "Dust in radio quiet quasars, ultra luminous infrared galaxies, radio galaxies and radio loud quasars." [S.l.] : [s.n.], 2001. http://deposit.ddb.de/cgi-bin/dokserv?idn=962893366.

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Tekola, Abiy G. "On the evolution of star forming galaxies : the metallicity of dwarfs and the effect of environment on local luminous IR galaxies." Doctoral thesis, University of Cape Town, 2011. http://hdl.handle.net/11427/11499.

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This thesis, entitled "On evolution of star forming galaxies: the metallicity of dwarfs and the effect of environment on local luminous infrared galaxies" is divided into two main areas. First a detailed study of the environment and star formation relationship of local Luminous Infrared Galaxies (LIRGs), with infrared (IR) luminosity (LIR) between 1011L and 1011L, where L is solar luminosity was carried out. Secondly, a chemical abundance analysis was done on three Local Volume dwarf irregular galaxies. In the first part, various redshift surveys were used to quantify the environment around LIRGs. It was found that LIR 1011L is a remarkable luminosity point among IR galaxies.
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Müller, Sven Archibald Hubertus [Verfasser]. "Dust in radio quiet quasars, ultra luminous infrared galaxies, radio galaxies and radio loud quasars / von Sven Archibald Hubertus Müller." 2001. http://d-nb.info/962893366/34.

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Book chapters on the topic "Ultra luminous IR galaxies"

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Scoville, Nick. "Ultra-Luminous IR Galaxies at Low and High Redshift." In Toward a New Millennium in Galaxy Morphology, 367–79. Dordrecht: Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-011-4114-7_28.

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Partridge, R. B., J. Marr, T. Crawford, and M. Strauss. "What Powers Ultra-Luminous IRAS Galaxies?" In Extragalactic Radio Sources, 215–16. Dordrecht: Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0295-4_76.

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Clements, D. L., A. C. Baker, and C. J. Lidman. "The Host Galaxies Of Ir Luminous Quasars." In Galaxy Interactions at Low and High Redshift, 350. Dordrecht: Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4665-4_85.

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Genzel, Reinhard, Dieter Lutz, Alan F. M. Moorwood, Dimitra Rigopoulou, Henrik W. W. Spoon, Amiel Sternberg, Eckhard Sturm, and Dan Tran. "The Nature of Ultra-Luminous Infrared Galaxies." In ISO Surveys of a Dusty Universe, 199–208. Berlin, Heidelberg: Springer Berlin Heidelberg, 2000. http://dx.doi.org/10.1007/3-540-45553-1_26.

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Gaffney, Niall I., Dan F. Lester, and Greg Doppmann. "Near-Infrared Measurements of Kinematics in Luminous Galaxies." In Spiral Galaxies in the Near-IR, 190–91. Berlin, Heidelberg: Springer Berlin Heidelberg, 1996. http://dx.doi.org/10.1007/978-3-540-49739-4_27.

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Gao, Y., R. A. Gruendl, C. Y. Hwang, and K. Y. Lo. "Luminous Ir Galaxies in a Merger Sequence: Bima Co Imaging." In Galaxy Interactions at Low and High Redshift, 227–30. Dordrecht: Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4665-4_55.

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Polatidis, A. G., J. E. Conway, Y. M. Pihlström, and R. Parra. "Continuum EVN and MERLIN Observations of Ultra Luminous Infrared Galaxies." In Dense Molecular Gas Around Protostars and in Galactic Nuclei, 297–302. Dordrecht: Springer Netherlands, 2005. http://dx.doi.org/10.1007/1-4020-3831-3_35.

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Alonso-Herrero, Almudena. "Near-IR Super Star Clusters in Starburst and Luminous Infrared Galaxies." In Starbursts, 35–40. Dordrecht: Springer Netherlands, 2005. http://dx.doi.org/10.1007/1-4020-3539-x_7.

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Väisänen, Petri, Zara Randriamanakoto, Stuart Ryder, and Seppo Mattila. "Super Star Clusters in IR-Luminous Interacting Galaxies: The NIR Luminosity Function." In Star Clusters in the Era of Large Surveys, 251–54. Berlin, Heidelberg: Springer Berlin Heidelberg, 2011. http://dx.doi.org/10.1007/978-3-642-22113-2_46.

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Aldering, G. "Uncovering Ultra-Luminous Galaxies in the IRAS FSC Through Radio and Optical Cross-Identification." In New Horizons from Multi-Wavelength Sky Surveys, 273–74. Dordrecht: Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-009-1485-8_61.

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Conference papers on the topic "Ultra luminous IR galaxies"

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Treister, Ezequiel. "Multiwavelength observations of ultra-luminous IR galaxies." In SUZAKU 2011: Exploring the X-ray Universe: Suzaku and Beyond. AIP, 2012. http://dx.doi.org/10.1063/1.3696177.

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Gao, Y., R. Gruendl, K. Y. Lo, C. Y. Hwang, and S. Veilleux. "Pre-starbursts in luminous IR galaxies?" In The seventh astrophysical conference: Star formation, near and far. AIP, 1997. http://dx.doi.org/10.1063/1.52748.

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Mühle, S. "The Search for Dense Gas in IR Luminous Galaxies." In THE EVOLUTION OF STARBURSTS: The 331st Wilhelm and Else Heraeus Seminar. AIP, 2005. http://dx.doi.org/10.1063/1.2034977.

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Iwasawa, K. "X-ray properties of ultra-luminous infrared galaxies (ULIGs)." In X-RAY ASTRONOMY: Stellar Endpoints,AGN, and the Diffuse X-ray Background. AIP, 2001. http://dx.doi.org/10.1063/1.1434630.

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Polatidis, A. G. "Continuum EVN and MERLIN Observations of Ultra Luminous Infrared Galaxies." In THE EVOLUTION OF STARBURSTS: The 331st Wilhelm and Else Heraeus Seminar. AIP, 2005. http://dx.doi.org/10.1063/1.2035006.

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Correa, Pablo, Rasha Abbasi, Markus Ackermann, Jenni Adams, Juanan Aguilar, M. Ahlers, Maryon Ahrens, et al. "IceCube Search for High-Energy Neutrinos from Ultra-Luminous Infrared Galaxies." In 37th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.1115.

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Raychaudhury, Somak, I. Mónica Vargas, Christine Jones, William R. Forman, Alexey Vikhlinin, Steve S. Murray, Sandip K. Chakrabarti, and Archan S. Majumdar. "The nature of Ultra-luminous X-ray sources in early-type galaxies." In OBSERVATIONAL EVIDENCE FOR BLACK HOLES IN THE UNIVERSE: Proceedings of the 2nd Kolkata Conference on Observational Evidence for Black Holes in the Universe held in Kolkata India, 10–15 February 2008 and the Satellite Meeting on Black Holes, Neutron Stars, and Gamma-Ray Bursts held 16–17 February 2008. AIP, 2008. http://dx.doi.org/10.1063/1.3009468.

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Correa, Pablo, Rasha Abbasi, Markus Ackermann, Jenni Adams, Juanan Aguilar, M. Ahlers, Maryon Ahrens, et al. "Searching for High-Energy Neutrinos from Ultra-Luminous Infrared Galaxies with IceCube." In The European Physical Society Conference on High Energy Physics. Trieste, Italy: Sissa Medialab, 2022. http://dx.doi.org/10.22323/1.398.0092.

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Borne, Kirk D. "A National Virtual Observatory (NVO) Science Case: Properties of Very Luminous IR Galaxies (VLIRGs)." In THE EMERGENCE OF COSMIC STRUCTURE: Thirteenth Astrophysics Conference. AIP, 2003. http://dx.doi.org/10.1063/1.1581808.

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Correa, Pablo, Krijn de Vries, and Nick van Eijndhoven. "Investigation of Ultra-Luminous Infrared Galaxies as Obscured High-Energy Neutrino Source Candidates." In 36th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0860.

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Reports on the topic "Ultra luminous IR galaxies"

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Mizuno, T. Accretion Disk Spectra of the Ultra-Luminous X-Ray Sources in Nearby Spiral Galaxies and Galactic Superluminal Jet Sources. Office of Scientific and Technical Information (OSTI), December 2003. http://dx.doi.org/10.2172/826596.

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