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Relevant bibliographies by topics / Interacting and isolated galaxies

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Academic literature on the topic 'Interacting and isolated galaxies'

Author: Grafiati

Published: 6 September 2023

Last updated: 31 July 2025

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Journal articles on the topic "Interacting and isolated galaxies"

1

Karachentsev, Igor D., Valentina E. Karachentseva, Walter K. Huchtmeier, Dmitry I. Makarov, and Serafim S. Kaisin. "Probe of Dark Galaxies via Disturbed/Lopsided Isolated Galaxies." Proceedings of the International Astronomical Union 3, S244 (2007): 235–46. http://dx.doi.org/10.1017/s1743921307014044.

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AbstractSearching for lopsided/interacting objects among 1500 isolated galaxies yields only eight strongly disturbed galaxies which may be explained as a result of their interaction with massive dark objects. We present results of spectral and photometric observations of these galaxies performed with the 6-m telescope that lead to significant restriction on cosmic abundance of dark galaxies.

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Struck, Curtis. "Star formation in mergers and interacting galaxies: gathering the fuel." Proceedings of the International Astronomical Union 2, S237 (2006): 317–22. http://dx.doi.org/10.1017/s1743921307001664.

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AbstractSelected results from recent studies of star formation in galaxies at different stages of interaction are reviewed. Recent results from the Spitzer Space Telescope are highlighted. Ideas on how large-scale driving of star formation in interacting galaxies might mesh with our understanding of star formation in isolated galaxies and small scale mechanisms within galaxies are considered. In particular, there is evidence that on small scales star formation is determined by the same thermal and turbulent processes in cool compressed clouds as in isolated galaxies. If so, this affirms the no

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Zaragoza-Cardiel, J., J. E. Beckman, J. Font, A. Camps-Fariña, B. García-Lorenzo, and S. Erroz-Ferrer. "Star formation enhancement characteristics in interacting galaxies." Proceedings of the International Astronomical Union 10, S309 (2014): 354. http://dx.doi.org/10.1017/s174392131401045x.

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AbstractWe have observed 12 interacting galaxies using the Fabry-Perot interferometer GHαFaS (Galaxy Hα Fabry-Perot system) on the 4.2m William Herschel Telescope (La Palma). We have extracted the physical properties (sizes, Hα luminosity and velocity dispersion) of 236 HII regions for the full sample of interacting galaxies. We have derived the physical properties of 664 HII regions for a sample of 28 isolated galaxies observed with the same instrument in order to compare both populations of HII regions, finding that there are brighter and denser star forming regions in the interacting galaxi

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Athanassoula, E. "Isolated and Interacting Galaxies: Simulations with GRAPE." Symposium - International Astronomical Union 208 (2003): 177–88. http://dx.doi.org/10.1017/s0074180900207134.

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I present N-body simulations of isolated and interacting galaxies, made on GRAPE machines. In particular I discuss the formation and evolution of N-body bars and compare their properties to those of bars in early-type and late-type galactic discs. I argue that the halo can help the bar grow, contrary to previous beliefs, by taking positive angular momentum from it via its resonant stars. I then focus on the interaction and subsequent merging of a barred disc galaxy with a spheroidal satellite. The evolution depends strongly on the mass (density) of the satellite and may lead to its destruction

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Kaneko, Hiroyuki, Nario Kuno, Daisuke Iono, et al. "Properties of molecular gas in galaxies in early and mid stages of Interaction. III. Resolved Kennicutt–Schmidt law." Publications of the Astronomical Society of Japan 74, no. 2 (2022): 343–63. http://dx.doi.org/10.1093/pasj/psab129.

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Abstract We study properties of the interstellar medium, an ingredient of stars, and star formation activity, in four nearby galaxy pairs in the early and mid stages of interaction for both a galaxy scale and a kpc scale. The galaxy-scale Kennicutt–Schmidt law shows that seven of eight interacting galaxies have a star formation rate within a factor of three compared with the best fit of the isolated galaxies, although we have shown that molecular hydrogen gas is efficiently produced from atomic hydrogen during the interaction in the previous paper (Kaneko et al. 2017 PASJ, 69, 66). The galaxy-

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Garay-Solis, Yeny, Jorge K. Barrera-Ballesteros, Dario Colombo, et al. "Exploring the Impact of Galactic Interactions and Mergers on the Central Star Formation of APEX/EDGE–CALIFA Galaxies." Astrophysical Journal 952, no. 2 (2023): 122. http://dx.doi.org/10.3847/1538-4357/acd781.

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Abstract Galactic interactions and subsequent mergers are a paramount channel for galaxy evolution. In this work, we use the data from 236 star-forming CALIFA galaxies with integrated molecular gas observations in their central region (approximately within an effective radius)—from the APEX millimeter telescope and the CARMA millimeter telescope array. This sample includes isolated (126 galaxies) and interacting galaxies in different merging stages (110 galaxies; from pairs, merging, and postmerger galaxies). We show that the impact of interactions and mergers in the center of galaxies is reve

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Fernández, María, Fangting Yuan, Shiyin Shen, Jun Yin, Ruixiang Chang, and Shuai Feng. "Isolated Galaxies versus Interacting Pairs with MaNGA." Galaxies 3, no. 4 (2015): 156–63. http://dx.doi.org/10.3390/galaxies3040156.

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Young, J. S. "Molecular Gas and Star Formation in Interacting and Isolated Galaxies." Symposium - International Astronomical Union 186 (1999): 217–26. http://dx.doi.org/10.1017/s0074180900112665.

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The results of the FCRAO Extragalactic CO Survey are used to examine the trends regarding the molecular gas distribution, the star formation efficiency, and the global gas surface densities (HI and H2) in galaxies as a function of environment. Relative to a sample of isolated Sbc-Scd galaxies, the strongly interacting galaxies have more compact gas distributions, a higher mean value for the global star formation efficiency, and a larger fraction of gas in molecular form. Not only is the molecular gas redistributed during interactions, but evidence is presented for an enhanced conversion of ato

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Bergvall, Nils, Eija Laurikainen, Susanne Aalto, and Lennart Johansson. "Star Formation in a Magnitude Limited Sample of Interacting Galaxies." Symposium - International Astronomical Union 171 (1996): 344. http://dx.doi.org/10.1017/s0074180900232634.

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We report on optical/near-IR spectroscopy and photometry of a magnitude limited sample of interacting pairs and merging galaxies and a control sample of apparently isolated galaxies (1,2). All observations were carried out at ESO, La Silla. When compared to the control sample, the interacting galaxies show only a moderate increase of star formation activity, in the central area typically a factor 2-3. Starburst activity seems to be very rare. Ongoing CO observations (Aalto, Horellou, Booth, Wiklind, Bergvall) indicate that these objects are not particularly rich in molecular gas. The interacti

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Lisenfeld, U., L. Verdes-Montenegro, J. Sulentic, et al. "The Far-Infrared Properties of the Most Isolated Galaxies." Proceedings of the International Astronomical Union 2, S235 (2006): 219. http://dx.doi.org/10.1017/s1743921306006259.

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AbstractWe describe the mid- (MIR) and far- (FIR) infrared properties of a large (~1000) sample of the most isolated galaxies in the local Universe. This sample is intended as a “nurture-free” zero point against which more environmentally influenced samples can be compared. We reprocess IRAS MIR/FIR survey data using the ADDSCAN/SCANPI utility for 1030 out of 1050 galaxies from the Catalogue of Isolated Galaxies (CIG) as part of the AMIGA project. We focus on diagnostics (FIR luminosity LFIR, R = log(LFIR/LB) and IRAS colours) thought to be sensitive to effects of environment or interaction. T

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Dissertations / Theses on the topic "Interacting and isolated galaxies"

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Kotarba, Hanna. "Magnetic Field Evolution in Isolated and Interacting Spiral Galaxies." Diss., lmu, 2011. http://nbn-resolving.de/urn:nbn:de:bvb:19-131513.

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Privon, G. C., S. Stierwalt, D. R. Patton, et al. "A Widespread, Clumpy Starburst in the Isolated Ongoing Dwarf Galaxy Merger dm1647+21." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/625751.

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Interactions between pairs of isolated dwarf galaxies provide a critical window into low-mass hierarchical, gas-dominated galaxy assembly and the build-up of stellar mass in low-metallicity systems. We present the first Very Large Telescope/Multi Unit Spectroscopic Explorer (VLT/MUSE) optical integral field unit (IFU) observations of the interacting dwarf pair dm1647+21 selected from the TiNy Titans survey. The Ha emission is widespread and corresponds to a total unobscured star formation rate (SFR) of 0.44 M-circle dot yr(-1), which is 2.7 times higher than the SFR inferred from Sloan Digital

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Reda, Fatma M. "Isolated elliptical galaxies." Swinburne Research Bank, 2007. http://hdl.handle.net/1959.3/20857.

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Thesis (Ph.D) - Swinburne University of Technology, Faculty of Information & Communication Technologies, 2007.<br>A thesis presented in fulfillment of the requirements of Doctor of Philosophy, Faculty of Information and Communication Technologies, Swinburne University of Technology, 2007. Typescript. Bibliography p. 109-118.

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Huang, S. N. "Dynamics of interacting galaxies." Thesis, University of Manchester, 1987. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.378332.

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Zhu, Ming. "Molecular gas in interacting galaxies." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 2001. http://www.collectionscanada.ca/obj/s4/f2/dsk3/ftp04/NQ58915.pdf.

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Cullen, H. E. "The physics of interacting galaxies." Thesis, University of Cambridge, 2005. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.598207.

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This thesis investigates interacting galaxies using two complementary approaches: a statistical study of star formation in a large sample of close pairs of galaxies drawn from the Sloan Digital Sky Survey (SDSS) and a study of the ISM and star forming properties of a small sample of interacting pairs taken from Arp’s atlas, each comprising one early- and one late-type system (E+S pairs). The first part of this thesis investigates the effect of galaxy interaction on star formation using a large volume- and luminosity-limited sample of galaxies drawn from the SDSS. Star-formation rates were calc

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Marston, A. P. "Observational aspects of interacting galaxies." Thesis, University of Manchester, 1987. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.382762.

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Wright, G. S. "Infrared activity in interacting galaxies." Thesis, Imperial College London, 1987. http://hdl.handle.net/10044/1/46917.

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Naab, Thorsten. "Structure and dynamics of interacting galaxies." [S.l. : s.n.], 2000. http://deposit.ddb.de/cgi-bin/dokserv?idn=961763744.

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Jonsson, Patrik. "Simulations of dust in interacting galaxies /." Diss., Digital Dissertations Database. Restricted to UC campuses, 2004. http://uclibs.org/PID/11984.

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Books on the topic "Interacting and isolated galaxies"

1

Read, Andrew Michael. High energy emission from isolated and interacting spiral galaxies. University of Birmingham, 1994.

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2

Zhu, Ming. Molecular gas in interacting galaxies. Graduate Department of Astronomy, University of Toronto, 2001.

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Johansson, Lennart. Activity in central parts of interacting parts of interacting galaxies. Uppsala Universitet, 1987.

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yliopisto, Turun, ed. Spectroscopy of a sample of interacting galaxies. University of Turku, 1989.

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5

Colloquium, International Astronomical Union. Paired and interacting galaxies: International Astronomical Union Colloquium no. 124. National Aeronautics and Space Administration, Office of Management, Scientific and Technical Information Division, 1990.

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6

John, Struck-Marcell Curtis, and United States. National Aeronautics and Space Administration., eds. Theoretical models of gas dymnamics in star formation in interacting ring galaxies: Final technical report. National Aeronautics and Space Administration, 1990.

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7

Sulentic, J. W. Paired and interacting galaxies: International Astronomical Union Colloquium No. 124 : proceedings of a conference sponsored by the International Astronomical Union, the University of Alabama at Tuscaloosa, and the National Aeronautics and Space Administration and held at the University of Alabama at Tuscaloosa, Tuscaloosa, Alabama, December 4-7, 1989. George C. Marshall Space Flight Center, 1990.

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Colloquium, International Astronomical Union. Paired and interacting galaxies: Proceedings of a conference sponsored by the International Astronomical Union, the University of Alabama at Tuscaloosa, and the National Aeronautics and Space Administration and held at the University of Alabama at Tuscaloosa, Alabama, December 4-7, 1989. National Aeronautics and Space Administration, Office of Management, Scientific and Technical Information Division, 1990.

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Colloquium, International Astronomical Union. Paired and interacting galaxies: Proceedings of a conference held at the University of Alabama at Tuscaloosa, Tuscaloosa, Alabama, December 4-7, 1989. NASA, Scientific and Technical Information Division, 1990.

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10

Chatzichristou, Eleni T. Imaging and Bidimensional Spectroscopy of Active and Interacting Galaxies. Self-published, 1999.

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Book chapters on the topic "Interacting and isolated galaxies"

1

Márquez, Isabel, Josefa Masegosa, Mariano Moles, Jesús Varela, Daniela Bettoni, and Giuseppe Galletta. "Isolated and Mildly Interacting Spiral Galaxies: Rotation Curves and Metallicities." In The Evolution of Galaxies. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-017-3315-1_80.

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Young, J. S. "Molecular Gas and Star Formation in Interacting And Isolated Galaxies." In Galaxy Interactions at Low and High Redshift. Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4665-4_54.

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Fuentes-Carrera, Isaura, Philippe Amram, and Margarita Rosado. "Dark Matter Haloes in Interacting Isolated Galaxy Pairs: The Importance of the Hα Rotation Curve." In The Evolution of Galaxies. Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-017-3311-3_94.

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Valtonen, Mauri, Joanna Anosova, Konstantin Kholshevnikov, Aleksandr Mylläri, Victor Orlov, and Kiyotaka Tanikawa. "Interacting Galaxies." In The Three-body Problem from Pythagoras to Hawking. Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-22726-9_6.

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Pisano, D. J., and Eric M. Wilcots. "Assembling Isolated Galaxies." In The Evolution of Galaxies. Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-017-3311-3_132.

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Verdes-Montenegro, L., M. Sauvage, M. J. Sempere, J. Sulentic, and J. Cernicharo. "Are Isolated Galaxies Boring?" In The Evolution of Galaxies. Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-017-3311-3_101.

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Davoust, E., Ph Prugniel, and J. Arnaud. "Interacting Pairs of Elliptical Galaxies." In The World of Galaxies. Springer US, 1989. http://dx.doi.org/10.1007/978-1-4613-9356-6_50.

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Combes, F., and A. L. Melchior. "Chemodynamical Evolution of Interacting Galaxies." In The Evolution of Galaxies. Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-017-3311-3_86.

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Noguchi, M. "Bar Formation in Interacting Galaxies." In Astrophysics and Space Science Library. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2917-3_61.

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Mihos, Chris. "Modeling Starbursts in Interacting Galaxies." In Starburst Galaxies: Near and Far. Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-642-56538-0_18.

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Conference papers on the topic "Interacting and isolated galaxies"

1

Sharma, Abhinav, Jeffrey Keller, and Glen Whitehouse. "A Fundamental Investigation of Ship Airwake Influence on Rotorcraft." In Vertical Flight Society 80th Annual Forum & Technology Display. The Vertical Flight Society, 2024. http://dx.doi.org/10.4050/f-0080-2024-1212.

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Rotorcraft responses to idealized disturbances are examined to gain insights into model fidelity requirements for flight simulations of the ship-rotorcraft dynamic interface. Two disturbance fields are considered: an isolated straight vortex that represents the canonical vortex that results from the corners of flat top ships in oblique wind-over-deck conditions and a horseshoe vortex derived from a nondimensional characterization of the time-averaged flow observed aft of a simplified ship superstructure. Rotorcraft models considered include: an analytical blade element theory-based rotor model

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Theis, Christian. "Starbursts in Isolated Galaxies?" In THE EVOLUTION OF STARBURSTS: The 331st Wilhelm and Else Heraeus Seminar. AIP, 2005. http://dx.doi.org/10.1063/1.2034967.

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Jonsson, Patrik. "Simulations of Dust in Interacting Galaxies." In THE SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data; International Workshop. AIP, 2005. http://dx.doi.org/10.1063/1.1913946.

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Petsch, H. P., A. Ružička, Ch Theis, Victor P. Debattista, and C. C. Popescu. "Measuring Dark Matter by Modeling Interacting Galaxies." In HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. AIP, 2010. http://dx.doi.org/10.1063/1.3458540.

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Lewin, Walter H. G. "X-ray sources in globular clusters of other galaxies." In INTERACTING BINARIES: Accretion, Evolution, and Outcomes. AIP, 2005. http://dx.doi.org/10.1063/1.2130211.

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Mengel, Sabine, Matthew D. Lehnert, Niranjan A. Thatte, and Reinhard Genzel. "Dynamical masses of young star clusters in interacting galaxies." In Astronomical Telescopes and Instrumentation, edited by Puragra Guhathakurta. SPIE, 2003. http://dx.doi.org/10.1117/12.456511.

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Lisenfeld, U. "The Role of Environment in Triggering Starburst Galaxies: A Sample of Isolated Galaxies." In THE EVOLUTION OF STARBURSTS: The 331st Wilhelm and Else Heraeus Seminar. AIP, 2005. http://dx.doi.org/10.1063/1.2034968.

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FRANCO-BALDERAS, A., E. BENÍTEZ, and J. A. DE DIEGO. "STUDY OF STELLAR POPULATIONS IN INTERACTING SYSTEMS OF SBS GALAXIES." In Proceedings of the Guillermo Haro Conference 2003. WORLD SCIENTIFIC, 2004. http://dx.doi.org/10.1142/9789812702432_0096.

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SIMONICH, J. "Isolated and interacting round parallel heated jets." In 24th Aerospace Sciences Meeting. American Institute of Aeronautics and Astronautics, 1986. http://dx.doi.org/10.2514/6.1986-281.

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Stella, L. "Young Rotation-Powered Pulsars as Ultraluminous X-ray Sources in Star-Forming Galaxies." In INTERACTING BINARIES: Accretion, Evolution, and Outcomes. AIP, 2005. http://dx.doi.org/10.1063/1.2130265.

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Reports on the topic "Interacting and isolated galaxies"

1

Chamovitz, Daniel A., and Zhenbiao Yang. Chemical Genetics of the COP9 Signalosome: Identification of Novel Regulators of Plant Development. United States Department of Agriculture, 2011. http://dx.doi.org/10.32747/2011.7699844.bard.

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This was an exploratory one-year study to identify chemical regulators of the COP9 signalosome. Chemical Genetics uses small molecules to modify or disrupt the function of specific genes/proteins. This is in contrast to classical genetics, in which mutations disrupt the function of genes. The underlying concept is that the functions of most proteins can be altered by the binding of a chemical, which can be found by screening large libraries for compounds that specifically affect a biological, molecular or biochemical process. In addition to screens for chemicals which inhibit specific biologic

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Clapham. L52206 3D Details of Defect-Induced MFL and Stress in Pipelines. Pipeline Research Council International, Inc. (PRCI), 2002. http://dx.doi.org/10.55274/r0011358.

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The following report represents a continuation of our ongoing efforts to understand and quantify the effect of stress on MFL signals from oil and gas transmission line inspection tools. Earlier GRI funding has enabled us to develop an unprecedented understanding of stress effects on magnetic behaviour in pipeline steels, and this understanding is now further enhanced and applied to specific problems such as MFL signals from interacting defects and also MFL signals produced from mechanical damage. This report summarizes the result of the 2002 studies. These studies focused on 3 main areas: MFL

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Or, Etti, Tai-Ping Sun, Amnon Lichter, and Avichai Perl. Characterization and Manipulation of the Primary Components in Gibberellin Signaling in the Grape Berry. United States Department of Agriculture, 2010. http://dx.doi.org/10.32747/2010.7592649.bard.

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Seedless cultivars dominate the table grape industry. In these cultivars it is mandatory to apply gibberellin (GA) to stimulate berry development to a commercially acceptable size. These cultivars differ in their sensitivity to GA application, and it frequently results in adverse effects such as decreased bud fertility and increased fruit drop. Our long term goals are to (1) understand the molecular basis for the differential sensitivity and identify markers for selection of sensitive cultivars (2) to develop new strategies for targeted manipulation of the grape berry response to GA that will

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