Relevant bibliographies by topics / Cooling flows (Astrophysics)

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters

Academic literature on the topic 'Cooling flows (Astrophysics)'

Author: Grafiati
Published: 4 June 2021
Last updated: 18 February 2022

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Journal articles on the topic "Cooling flows (Astrophysics)"

1

Kley, Wilhelm, and William G. Mathews. "Rotating cooling flows." Astrophysical Journal 438 (January 1995): 100. http://dx.doi.org/10.1086/175057.

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Nulsen, P. E. J. "Isothermal cooling flows." Monthly Notices of the Royal Astronomical Society 297, no. 4 (July 11, 1998): 1109–14. http://dx.doi.org/10.1046/j.1365-8711.1998.29741109.x.

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3

Brighenti, Fabrizio, and William G. Mathews. "Heated Cooling Flows." Astrophysical Journal 573, no. 2 (July 10, 2002): 542–61. http://dx.doi.org/10.1086/340763.

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Donahue, Megan, John T. Stocke, and Isabella M. Gioia. "Distant cooling flows." Astrophysical Journal 385 (January 1992): 49. http://dx.doi.org/10.1086/170914.

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Binney, J., and G. Tabor. "Evolving cooling flows." Monthly Notices of the Royal Astronomical Society 276, no. 2 (September 15, 1995): 663–78. http://dx.doi.org/10.1093/mnras/276.2.663.

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Mathews, William G., Fabrizio Brighenti, David A. Buote, and Aaron D. Lewis. "Circulation Flows: Cooling Flows with Bubble Return." Astrophysical Journal 596, no. 1 (October 10, 2003): 159–69. http://dx.doi.org/10.1086/377596.

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Westbury, Catherine F., and R. N. Henriksen. "Turbulence in cooling flows." Astrophysical Journal 388 (March 1992): 64. http://dx.doi.org/10.1086/171130.

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Salomé, Philippe. "Brightest Cluster Galaxies & Cooling Flows." Proceedings of the International Astronomical Union 8, S292 (August 2012): 169–74. http://dx.doi.org/10.1017/s1743921313000975.

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AbstractIn the absence of any form of feedback heating, the gas in the central regions of massive relaxed cluster should cool and initiate a cooling flow. The presence/efficiency of an additional heating and the ultimate fate of the cooling gas is the subject of an extensive debate. In the last decade, molecular and atomic gas have been found in many Brightest Cluster Galaxies. I will review these observational results and discuss their implication for galaxy formation/evolution, in the perspective of ALMA.
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Mirabel, I. F. "High Velocity OH in Bipolar Flows." Symposium - International Astronomical Union 115 (1987): 315–23. http://dx.doi.org/10.1017/s0074180900095668.

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High velocity OH was detected in absorption in several star forming regions. The supersonic OH shows similar bipolar geometry as the CO. The absorbing OH appears to trace the part of the outflows with the highest velocities and lower densities, and provides information on the structure of the outflows at large distances from the central source. At scales of 0.1 to 0.5 parsecs the outflows are elongated in the direction of the steepest density gradient in the ambient cloud. The transitions in the supersonic OH are markedly subthermal (Tex < 3.8 K), since the radiation that is being absorbed is the cosmic background plus a small galactic contribution. We propose a cooling mechanism for the OH analogous to the adiabatic magnetic cooling of paramagnetic salts used in low temperature physics. Magnetic cooling is a potentially important mechanism for astrophysics.
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Pavlovski, Georgi, and Edward C. D. Pope. "Stochastic heating of cooling flows." Monthly Notices of the Royal Astronomical Society 399, no. 4 (November 11, 2009): 2195–200. http://dx.doi.org/10.1111/j.1365-2966.2009.15424.x.

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Dissertations / Theses on the topic "Cooling flows (Astrophysics)"

1

Thomas, Peter Andrew. "Cooling flows and galaxy formation." Thesis, University of Cambridge, 1987. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.329135.

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Pilorz, Stuart. "Galactic winds and cooling flows." Thesis, University of Oxford, 1997. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.242035.

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Tabor, Gavin R. "New models of galactic cooling flows." Thesis, University of Oxford, 1994. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.358712.

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Daines, Stuart. "Cooling flows and cold gas in clusters of galaxies." Thesis, University of Cambridge, 1994. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.321020.

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Arnaud, K. A. "X-ray emitting gas, cooling flows and stellar populations in elliptical galaxies." Thesis, University of Cambridge, 1985. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.355666.

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Diehl, Steven. "The Hot Interstellar Medium in Normal Elliptical Galaxies." Ohio University / OhioLINK, 2006. http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1149262336.

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Rafferty, David A. "Feedback in Cluster Cores." Ohio University / OhioLINK, 2007. http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1186765820.

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8

Salome, Philippe. "Le gaz moleculaire dans les galaxies abritant un courant de refroidissement." Phd thesis, Université Paris Sud - Paris XI, 2004. http://tel.archives-ouvertes.fr/tel-00338287.

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Les prédictions théoriques de refroidissement du gaz intra-amas depuis des températures de 10^7 K jusqu'à une phase très froide n'ont jamais été prouvées directement. L'apport des satellites Chandra et XMM-Newton a permis de mieux sonder le centre de certaines de ces grandes structures, où le courant de refroidissement a lieu. Un problème majeur est la question du devenir du gaz refroidi. Le travail présenté ici est la détection de gaz moléculaire au centre de plusieurs amas de galaxies, obtenues avec le télescope de 30m de l'IRAM. Ces détections vont dans le sens d'une possible identification du composant froid directement issu du courant de refroidissement. La quantité de gaz moléculaire estimée reste toutefois encore inférieure à ce que prévoient les taux de déposition de masse déduits de l'émission du gaz chaud. Afin de mieux comprendre l'origine de ce composant froid, une étude plus précise d'un amas particulier : Abell 1795 a été menée. L'analyse spectrale des données X du satellite Chandra a permis de dériver des propriétés importantes du gaz chaud (température, abondance, colonne densité, taux de déposition de masse). Pour comprendre le lien entre le gaz moléculaire et le courant de refroidissement, des observations en CO(1-0) et CO(2-1) d'Abell 1795 ont été menées avec l'interféromètre du Plateau de Bure (IRAM). La morphologie et la dynamique du gaz froid sont apparemment associées à celles des composants plus chauds. Ces observations sont donc compatibles avec un refroidissement du gaz jusqu'à très basse température, fournissant un réservoir de matière disponible pour nourrir la formation stellaire effectivement active au centre de l'amas. De nouvelles contraintes observationnelles sont maintenant envisagées (Plateau de Bure, VLT) sur un plus large échantillon pour tenter de comprendre plus clairement la place du gaz moléculaire, dans un scénario de courant de refroidissement où les processus de réchauffement sont certainement actifs.
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Books on the topic "Cooling flows (Astrophysics)"

1

NATO, Advanced Research Workshop on Cooling Flows in Clusters and Galaxies (1987 Cambridge England). Cooling flows in clusters and galaxies. Dordrecht: Kluwer Academic Publishers, 1988.

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2

Stone, James M. The stability of radiatively cooling jets. [Washington, DC: National Aeronautics and Space Administration, 1997.

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3

United States. National Aeronautics and Space Administration., ed. The mass and dynamics of cD clusters with cooling flows. [Washington, DC: National Aeronautics and Space Administration, 1994.

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4

Stephen, Dillingham, and United States. National Aeronautics and Space Administration., eds. A study of cooling flows in poor clusters of galaxies. [Washington, D.C: National Aeronautics and Space Administration, 1995.

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5

United States. National Aeronautics and Space Administration., ed. X-Ray spectroscopy of cooling flows: NASA grant NAG5-2607, final report for the period 1 June 1994 through 30 November 1995. Cambridge, Mass: Smithsonian Institution, Astrophysical Observatory, 1996.

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6

United States. National Aeronautics and Space Administration., ed. X-Ray spectroscopy of cooling flows: NASA grant NAG5-2607, final report for the period 1 June 1994 through 30 November 1995. Cambridge, Mass: Smithsonian Institution, Astrophysical Observatory, 1996.

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7

X-Ray spectroscopy of cooling flows: NASA grant NAG5-2607, final report for the period 1 June 1994 through 30 November 1995. Cambridge, Mass: Smithsonian Institution, Astrophysical Observatory, 1996.

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United States. National Aeronautics and Space Administration., ed. X-Ray spectroscopy of cooling flows: NASA grant NAG5-2607, final report for the period 1 June 1994 through 30 November 1995. Cambridge, Mass: Smithsonian Institution, Astrophysical Observatory, 1996.

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Book chapters on the topic "Cooling flows (Astrophysics)"

1

Mushotzky, Richard. "Cooling Flows in Clusters of Galaxies." In Astrophysics and Space Science Library, 383–408. Dordrecht: Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-1882-8_22.

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2

Rafferty, D. A., B. R. McNamara, P. E. J. Nulsen, and M. W. Wise. "The Growth of Black Holes and Bulges at the Cores of Cooling Flows." In Eso Astrophysics Symposia, 121–23. Berlin, Heidelberg: Springer Berlin Heidelberg, 2007. http://dx.doi.org/10.1007/978-3-540-73484-0_23.

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Fujita, Y., and T. Ken Suzuki. "The Difficulty of the Heating of Cluster Cooling Flows by Sound Waves and Weak Shocks." In Eso Astrophysics Symposia, 216–21. Berlin, Heidelberg: Springer Berlin Heidelberg, 2007. http://dx.doi.org/10.1007/978-3-540-73484-0_38.

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4

Pizzolato, F. "Cold Feedback in Cooling–Flow Galaxy Clusters." In Eso Astrophysics Symposia, 243–47. Berlin, Heidelberg: Springer Berlin Heidelberg, 2007. http://dx.doi.org/10.1007/978-3-540-73484-0_44.

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Revaz, Y., F. Combes, and F. Salomé. "Formation of Cold Molecular Filaments in Cooling Flow Flusters." In Eso Astrophysics Symposia, 330–32. Berlin, Heidelberg: Springer Berlin Heidelberg, 2007. http://dx.doi.org/10.1007/978-3-540-73484-0_60.

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Vikhlinin, A., R. Burenin, W. R. Forman, C. Jones, A. Hornstrup, S. S. Murray, and H. Quintana. "Lack of Cooling Flow Clusters at z > 0.5." In Eso Astrophysics Symposia, 48–53. Berlin, Heidelberg: Springer Berlin Heidelberg, 2007. http://dx.doi.org/10.1007/978-3-540-73484-0_9.

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7

Mondal, Santanu. "Transonic Flow Solutions with Explicit Cooling and Viscosity." In Astrophysics and Space Science Proceedings, 67–83. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-94607-8_6.

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Nesci, R., G. C. Perola, I. M. Gioica, T. Maccacaro, R. E. Schild, and A. Wolter. "A Distant X-Ray Selected Cluster with a Cooling Flow: 1E0839.9+2938." In Astrophysics and Space Science Library, 413–14. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0903-8_70.

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