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Books on the topic 'Interacting and isolated galaxies'

Author: Grafiati

Published: 6 September 2023

Last updated: 31 July 2025

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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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3

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

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4

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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8

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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9

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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11

The search for extended infrared emission near interacting and active galaxies. National Aeronautics and Space Administration, 1991.

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12

[IRAS high resolution studies and modeling of closely interacting galaxies: Galaxy collisions:infrared observations and analysis of numerical models and UV spectroscopy of massive young stellar populations in interacting galaxies]. National Aeronautics and Space Administration, 1993.

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13

National Aeronautics and Space Administration (NASA) Staff. Iras High Resolution Studies and Modeling of Closely Interacting Galaxies. Galaxy Collisions: Infrared Observations and Analysis of Numerical Models. UV Spectroscopy of Massive Young Stellar Populations in Interacting Galaxies. Independently Published, 2018.

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14

Woods, Deborah Freedman. Tidally triggered star formation in gravitationally interacting galaxies and selected work in optical instrumentation. 2009.

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15

Sulentic, J. E. Paired and Interacting Galaxies Conference Summary of the International Astronomical Union Colloquium No 124 in Tuluksak, Alabama, Dec. 4-7, 1989. Natl Technical Information, 1991.

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16

Galaxy wars: Stellar populations and star formation in interacting galaxies : proceedings of a conference held at East Tennessee State University, Johnson City, Tennessee, USA, 19-22 July 2009. Astronomical Society of the Pacific, 2010.

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17

Kobayashi, Shiro, Soo-Ik Oh, and Taylan Altan. Metal Forming and the Finite-Element Method. Oxford University Press, 1989. http://dx.doi.org/10.1093/oso/9780195044027.001.0001.

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The application of computer-aided design and manufacturing techniques is becoming essential in modern metal-forming technology. Thus process modeling for the determination of deformation mechanics has been a major concern in research . In light of these developments, the finite element method--a technique by which an object is decomposed into pieces and treated as isolated, interacting sections--has steadily assumed increased importance. This volume addresses advances in modern metal-forming technology, computer-aided design and engineering, and the finite element method.

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18

EX56a study of extended X-ray emission around isolated galaxies : EX56b identification and spectra of bright X-ray sources at high galactic latitude: Final report for the period 1 April 1985 through 30 November 1986. National Aeronautics and Space Administration, 1987.

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19

Mashhoon, Bahram. Nonlocal Gravity and Dark Matter. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780198803805.003.0008.

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The implications of linearized NLG for the gravitational physics of the Solar System, spiral galaxies and nearby clusters of galaxies are critically examined in this chapter. In the Newtonian regime, NLG involves a reciprocal kernel with three length parameters. We discuss the determination of these parameters by comparing the predictions of the theory with observational data. Furthermore, the virial theorem for the Newtonian regime of NLG is derived and its consequences for nearby “isolated” astronomical systems in virial equilibrium are investigated. For such a galaxy, in particular, the gal

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20

Lurcock, Pontus, and Fabio Florindo. Antarctic Climate History and Global Climate Changes. Oxford University Press, 2017. http://dx.doi.org/10.1093/oxfordhb/9780190676889.013.18.

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Antarctic climate changes have been reconstructed from ice and sediment cores and numerical models (which also predict future changes). Major ice sheets first appeared 34 million years ago (Ma) and fluctuated throughout the Oligocene, with an overall cooling trend. Ice volume more than doubled at the Oligocene-Miocene boundary. Fluctuating Miocene temperatures peaked at 17–14 Ma, followed by dramatic cooling. Cooling continued through the Pliocene and Pleistocene, with another major glacial expansion at 3–2 Ma. Several interacting drivers control Antarctic climate. On timescales of 10,000–100,

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21

Lurcock, Pontus, and Fabio Florindo. Antarctic Climate History and Global Climate Changes. Oxford University Press, 2017. http://dx.doi.org/10.1093/oxfordhb/9780190699420.013.18.

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Antarctic climate changes have been reconstructed from ice and sediment cores and numerical models (which also predict future changes). Major ice sheets first appeared 34 million years ago (Ma) and fluctuated throughout the Oligocene, with an overall cooling trend. Ice volume more than doubled at the Oligocene-Miocene boundary. Fluctuating Miocene temperatures peaked at 17–14 Ma, followed by dramatic cooling. Cooling continued through the Pliocene and Pleistocene, with another major glacial expansion at 3–2 Ma. Several interacting drivers control Antarctic climate. On timescales of 10,000–100,

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22

Hoff, Timothy J. Next in Line. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780190626341.001.0001.

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The doctor-patient relationship is besieged by several forces transforming the health care system at the present time, particularly the introduction of retail thinking that seeks to turn patients into consumers. This book examines how the relationship has changed and continues to evolve within a care delivery context that is more corporatized, value-driven, metric-oriented, and transactional than ever before. Through the voices of doctors and patients, combined with an in-depth analysis of bigger system trends, it finds that relational care characterized by proven interpersonal and humane feat

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