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Books on the topic 'Interacting and isolated galaxies'

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Published: 6 September 2023

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1

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

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2

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

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3

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

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4

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. [Washington, DC]: National Aeronautics and Space Administration, 1990.

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5

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. Marshall Space Flight Center, Ala: George C. Marshall Space Flight Center, 1990.

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6

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. Washington, D.C: National Aeronautics and Space Administration, Office of Management, Scientific and Technical Information Division, 1990.

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7

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. [Washington, D.C.]: NASA, Scientific and Technical Information Division, 1990.

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8

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. San Francisco: Astronomical Society of the Pacific, 2010.

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9

The search for extended infrared emission near interacting and active galaxies. [Washington, D.C.?: National Aeronautics and Space Administration, 1991.

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10

[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]. [Washington, DC: National Aeronautics and Space Administration, 1993.

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11

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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12

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

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13

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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14

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. [Washington, DC: National Aeronautics and Space Administration, 1987.

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15

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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16

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 galaxy’s baryonic diameter namely, the diameter of the smallest sphere that completely surrounds the baryonic system at the present time, is predicted to be larger than the basic nonlocality lengthscale, which is about 3 kpc, times the effective dark matter fraction of the galaxy.
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17

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 10,000–100,000 years, insolation varies with orbital cycles, causing periodic climate variations. Opening of Southern Ocean gateways produced a circumpolar current that thermally isolated Antarctica. Declining atmospheric CO2 triggered Cenozoic glaciation. Antarctic glaciations affect global climate by lowering sea level, intensifying atmospheric circulation, and increasing planetary albedo. Ice sheets interact with ocean water, forming water masses that play a key role in global ocean circulation.
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18

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 10,000–100,000 years, insolation varies with orbital cycles, causing periodic climate variations. Opening of Southern Ocean gateways produced a circumpolar current that thermally isolated Antarctica. Declining atmospheric CO2 triggered Cenozoic glaciation. Antarctic glaciations affect global climate by lowering sea level, intensifying atmospheric circulation, and increasing planetary albedo. Ice sheets interact with ocean water, forming water masses that play a key role in global ocean circulation.
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19

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 features like trust, empathy, and mutual respect has withered over time, succumbing to a hostile delivery environment in which physicians are increasingly isolated from patients; the organization seeks to garner the allegiances of patients; and patients develop lowered expectations that leave them susceptible to cheapened forms of care delivery. Both doctors and patients still emphasize the importance of relational care for effective diagnosis and treatment, and for maintaining strong emotional bonds that enhance both parties’ experiences. However, the findings suggest that the rise of transactional care delivery in the health system must be offset by greater physician advocacy for relational medicine; a sharp focus on measuring relational care delivery in all its forms; and monetizing relational care so that it becomes something of value to the large organizations in which doctors and patients now find themselves interacting.
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