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

Author: Grafiati

Published: 4 June 2021

Last updated: 18 February 2022

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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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2

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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4

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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5

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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6

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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7

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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8

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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9

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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10

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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11

Sparks, W. B. "Mergers, cooling flows, and evaporation." Astrophysical Journal 399 (November 1992): 66. http://dx.doi.org/10.1086/171903.

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12

Henriksen, Mark J. "Cooling flows and cluster evolution." Astrophysical Journal 407 (April 1993): L13. http://dx.doi.org/10.1086/186794.

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13

Omma, Henrik, and James Binney. "Structural stability of cooling flows." Monthly Notices of the Royal Astronomical Society 350, no. 1 (May 2004): L13—L16. http://dx.doi.org/10.1111/j.1365-2966.2004.07809.x.

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14

Colafrancesco, S., Arnon Dar, and A. De Rújula. "Cooling flows or warming rays?" Astronomy & Astrophysics 413, no. 2 (December 18, 2003): 441–52. http://dx.doi.org/10.1051/0004-6361:20031509.

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15

Brighenti, Fabrizio, and William G. Mathews. "Stopping Cooling Flows with Jets." Astrophysical Journal 643, no. 1 (May 20, 2006): 120–27. http://dx.doi.org/10.1086/502645.

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16

Nulsen, P. E. J. "Thermal instability in cooling flows." Monthly Notices of the Royal Astronomical Society 221, no. 2 (July 1, 1986): 377–92. http://dx.doi.org/10.1093/mnras/221.2.377.

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17

Buote, David A. "Oxygen Absorption in Cooling Flows." Astrophysical Journal 532, no. 2 (April 1, 2000): L113—L116. http://dx.doi.org/10.1086/312580.

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18

Bregman, Joel N., and L. P. David. "Alternative models of cooling flows." Astrophysical Journal 341 (June 1989): 49. http://dx.doi.org/10.1086/167470.

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19

Loewenstein, Michael. "Magnetothermal instability in cooling flows." Astrophysical Journal 349 (February 1990): 471. http://dx.doi.org/10.1086/168331.

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20

Bregman, Joel N., and L. P. David. "Heat conduction in cooling flows." Astrophysical Journal 326 (March 1988): 639. http://dx.doi.org/10.1086/166122.

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21

Brighenti, Fabrizio, and William G. Mathews. "Where Do Cooling Flows Cool?" Astrophysical Journal 535, no. 2 (June 2000): 650–62. http://dx.doi.org/10.1086/308858.

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22

Bertschinger, Edmund. "The evolution of cooling flows - Self-similar cooling waves." Astrophysical Journal 340 (May 1989): 666. http://dx.doi.org/10.1086/167428.

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23

Fabian, A. C., C. R. Canizares, and H. Boehringer. "Mergers, cooling flows, and evaporation revisited." Astrophysical Journal 425 (April 1994): 40. http://dx.doi.org/10.1086/173959.

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24

Gómez, P. L., C. Loken, K. Roettiger, and J. O. Burns. "Do Cooling Flows Survive Cluster Mergers?" Astrophysical Journal 569, no. 1 (April 2002): 122–33. http://dx.doi.org/10.1086/339280.

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25

Jaffe, W., and M. N. Bremer. "Molecular hydrogen emission in cooling flows." Monthly Notices of the Royal Astronomical Society 284, no. 1 (January 1, 1997): L1—L5. http://dx.doi.org/10.1093/mnras/284.1.l1.

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26

Mathews, William G., and Fulai Guo. "RADIATING BONDI AND COOLING SITE FLOWS." Astrophysical Journal 754, no. 2 (July 18, 2012): 154. http://dx.doi.org/10.1088/0004-637x/754/2/154.

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27

Myers, P. C., and A. Lazarian. "Turbulent Cooling Flows in Molecular Clouds." Astrophysical Journal 507, no. 2 (November 10, 1998): L157—L160. http://dx.doi.org/10.1086/311700.

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28

Fabian, A. C., P. E. J. Nulsen, and C. R. Canizares. "Cooling flows in clusters of galaxies." Astronomy and Astrophysics Review 2, no. 3-4 (1991): 191–226. http://dx.doi.org/10.1007/bf00872767.

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29

Chevalier, Roger A. "The evolution of cooling flows. I - Self-similar cluster flows." Astrophysical Journal 318 (July 1987): 66. http://dx.doi.org/10.1086/165351.

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30

Mathews, William G., Fabrizio Brighenti, and David A. Buote. "Time‐dependent Circulation Flows: Iron Enrichment in Cooling Flows with Heated Return Flows." Astrophysical Journal 615, no. 2 (November 10, 2004): 662–74. http://dx.doi.org/10.1086/424705.

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31

Donahue, Megan, and John T. Stocke. "Coronal line emission in cluster cooling flows." Astrophysical Journal 422 (February 1994): 459. http://dx.doi.org/10.1086/173741.

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32

Bregman, Joel N., Eric D. Miller, Alex E. Athey, and Jimmy A. Irwin. "Oviin Elliptical Galaxies: Indicators of Cooling Flows." Astrophysical Journal 635, no. 2 (December 20, 2005): 1031–43. http://dx.doi.org/10.1086/497421.

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33

Mathews, William G., Andreas Faltenbacher, and Fabrizio Brighenti. "Heating Cooling Flows with Weak Shock Waves." Astrophysical Journal 638, no. 2 (February 20, 2006): 659–67. http://dx.doi.org/10.1086/499119.

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34

O'Connell, Robert W., and Brian R. McNamara. "The Fate of Matter in Cooling Flows." Astronomical Journal 98 (July 1989): 180. http://dx.doi.org/10.1086/115135.

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35

Molendi, Silvano, and Fabio Pizzolato. "Is the Gas in Cooling Flows Multiphase?" Astrophysical Journal 560, no. 1 (October 10, 2001): 194–200. http://dx.doi.org/10.1086/322387.

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36

De Young, D. S. "Relic radio 'bubbles' and cluster cooling flows." Monthly Notices of the Royal Astronomical Society 343, no. 3 (August 11, 2003): 719–24. http://dx.doi.org/10.1046/j.1365-8711.2003.06719.x.

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37

Mathews, William G. "STOPPING COOLING FLOWS WITH COSMIC-RAY FEEDBACK." Astrophysical Journal 695, no. 1 (March 23, 2009): L49—L52. http://dx.doi.org/10.1088/0004-637x/695/1/l49.

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38

Tribble, P. C. "Radio haloes, cluster mergers, and cooling flows." Monthly Notices of the Royal Astronomical Society 263, no. 1 (July 1, 1993): 31–36. http://dx.doi.org/10.1093/mnras/263.1.31.

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39

Soker, Noam, Joel N. Bregman, and Craig L. Sarazin. "Stripped interstellar gas in cluster cooling flows." Astrophysical Journal 368 (February 1991): 341. http://dx.doi.org/10.1086/169698.

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40

Balbus, Steven A. "On magnetothermal instability in cluster cooling flows." Astrophysical Journal 372 (May 1991): 25. http://dx.doi.org/10.1086/169951.

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41

Voit, G. Mark, and Megan Donahue. "Problems with Cold Clouds and Cooling Flows." Astrophysical Journal 452 (October 1995): 164. http://dx.doi.org/10.1086/176288.

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42

Norman, Colin, and Avery Meiksin. "Two-Phase Cooling Flows with Magnetic Reconnection." Astrophysical Journal 468 (September 1996): 97. http://dx.doi.org/10.1086/177673.

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43

Ciotti, Luca, and Jeremiah P. Ostriker. "Cooling Flows and Quasars. II. Detailed Models of Feedback‐modulated Accretion Flows." Astrophysical Journal 551, no. 1 (April 10, 2001): 131–52. http://dx.doi.org/10.1086/320053.

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44

Donahue, Megan, and John T. Stocke. "Coronal Line Emission in Cluster Cooling Flows: Erratum." Astrophysical Journal 446 (June 1995): 909. http://dx.doi.org/10.1086/175849.

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45

Mathews, William G., and Fabrizio Brighenti. "Self‐generated Magnetic Fields in Galactic Cooling Flows." Astrophysical Journal 488, no. 2 (October 20, 1997): 595–605. http://dx.doi.org/10.1086/304728.

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46

Shadmehri, Mohsen, and Jamshid Ghanbari. "Cooling Flows of Self‐gravitating, Rotating, Viscous Systems." Astrophysical Journal 574, no. 1 (July 20, 2002): 198–204. http://dx.doi.org/10.1086/340894.

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47

McCarthy, Ian G., Arif Babul, Neal Katz, and Michael L. Balogh. "On the Relationship between Cooling Flows and Bubbles." Astrophysical Journal 587, no. 2 (March 20, 2003): L75—L78. http://dx.doi.org/10.1086/375336.

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48

Tabor, Gavin, and James Binney. "Elliptical galaxy cooling flows without mass drop-out." Monthly Notices of the Royal Astronomical Society 263, no. 2 (July 1993): 323–34. http://dx.doi.org/10.1093/mnras/263.2.323.

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49

Johnstone, R. M., and A. C. Fabian. "Cooling flows and a giant red envelope galaxy." Monthly Notices of the Royal Astronomical Society 237, no. 1 (March 1989): 27P—30P. http://dx.doi.org/10.1093/mnras/237.1.27p.

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50

Loewenstein, M. "Evolution of overdense regions in cluster cooling flows." Monthly Notices of the Royal Astronomical Society 238, no. 1 (May 1989): 15–41. http://dx.doi.org/10.1093/mnras/238.1.15.

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