Skip to main content Accessibility help
×
Hostname: page-component-848d4c4894-wzw2p Total loading time: 0 Render date: 2024-05-03T21:39:21.113Z Has data issue: false hasContentIssue false

12 - Magnetic fields in cosmologically distant galaxy systems

Published online by Cambridge University Press:  22 September 2016

Philipp P. Kronberg
Affiliation:
University of Toronto
Get access

Summary

Image of the first page of this content. For PDF version, please use the ‘Save PDF’ preceeding this image.'
Type
Chapter
Information
Publisher: Cambridge University Press
Print publication year: 2016

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Bell, A. R. 1978, The Acceleration of Cosmic Rays in Shock Fronts. I, MNRAS, 182, 147CrossRefGoogle Scholar
Bernet, M. L., Miniati, F., Lilly, S. J., Kronberg, P. P., & Dessauges-Zavadsky, M. 2008, Strong Magnetic Fields in Normal Galaxies at High Redshift, Nature, 454, 302CrossRefGoogle ScholarPubMed
Biermann, L. 1950, Über den Ursprung der Magnetfelder auf Sternen und im interstellaren Raum (mit einem Anhang von A. Schlüter), Zeitschrift für Astrophysik, 5a, 65Google Scholar
Blandford, R. D. & Narayan, R. 1992, Cosmological Applications of Gravitational Lensing, Ann. Rev. Ast. Astrophys., 30, 311CrossRefGoogle Scholar
Braun, R., Heald, G., & Beck, R. 2010, The Westerbork SINGS Survey. III. Global Magnetic Field Topology, Astron. Astrophys., 514, 42CrossRefGoogle Scholar
Burbidge, G. R., O’Dell, S. L., Roberts, D. H., & Smith, H. E. 1977, On the Origin of the Absorption Spectra of Quasistellar and BL Lacertae Objects, Astrophys. J., 218, 33CrossRefGoogle Scholar
Cen, R. & Ostriker, J. P. 1999, Where Are the Baryons?, Astrophys. J., 514, 1CrossRefGoogle Scholar
Chen, G. H. & Hewitt, J. N. 1993, Multifrequency Radio Images of the Einstein Ring Gravitational Lens MG 1131+0456, Astron. J., 106, 1719CrossRefGoogle Scholar
Cho, J. & Vishniac, E. T. 2000, The Generation of Magnetic Fields through Driven Turbulence, Astrophys J., 538, 217CrossRefGoogle Scholar
Dickey, J. M. & Salpeter, E. E. 1984, 1.4 GHz Continuum Sources in the Hercules Cluster, Astron. J., 284, 461CrossRefGoogle Scholar
Dieckmann, M. E., Shukla, P. K., & Drury, L. O. C. 2008, The Formation of a Relativistic Partially Electromagnetic Planar Plasma Shock, Astrophys J., 675, 586CrossRefGoogle Scholar
Dyer, C. C. & Roeder, R. C. 1977, Optical Scalars and the Spherical Gravitational Lens, MNRAS., 180, 231CrossRefGoogle Scholar
Dyer, C. C. & Shaver, E. G. 1992, On the Rotation of Polarisation by a Gravitational Lens, Astrophys. J. Lett., 390, L5CrossRefGoogle Scholar
Elstner, D., Meinel, R., & Beck, R. 1992, Galactic Dynamos and Their Radio Signatures, Astron. Astrophys. Suppl. Ser., 94, 587Google Scholar
Elstner, D., Otmianowska-Mazur, K., von Linden, S., & Urbanik, M. 2000, Galactic Magnetic Fields and Spiral Arms. 3D Dynamo Simulations, Astron. Astrophys., 357, 129Google Scholar
Foltz, C. B., Chaffee, F. H., Weymann, R. J., & Anderson, S. F. 1988, QSO Absorption Systems with Z(ABS) = about Z(EM), in QSO Absorption Lines: Probing the Universe; Proceedings of the QSO Absorption Line Meeting, Baltimore, MD, May 19–21, 1987 (Cambridge; New York: Cambridge University Press), 53Google Scholar
Garrington, S. T. & Conway, R. G. 1991, The Interpretation of Asymmetric Depolarization in Extragalactic Radio Sources, MNRAS, 250, 198CrossRefGoogle Scholar
Gnedin, Y., Ferrara, A., & Zweibel, E. N. 2000, Generation of the Primordial Magnetic Fields during Cosmological Reionization, Astrophys. J., 539, 505CrossRefGoogle Scholar
Grasso, D. & Rubenstein, H. R. 2001, Magnetic Fields in the Early Universe, Phys. Rep., 348, 163CrossRefGoogle Scholar
Gruzinov, A. 2001, Gamma-Ray Burst Phenomenology, Shock Dynamo, and the First Magnetic Fields, Astrophys. J., 563, L15CrossRefGoogle Scholar
Harwit, M. & Pacini, F. 1975, Astrophys. J., 200, L127CrossRefGoogle Scholar
Hazard, C., MacKay, M. B., & Shimmins, A. J. 1963, Investigation of the Radio Source 3C 273 by the Method of Lunar Occultations, Nature, 197, 1037CrossRefGoogle Scholar
Helou, G., Soifer, B. T. & Rowan-Robinson, M. 1985, Thermal Infrared and Nonthermal Radio – Remarkable Correlation in Disks of Galaxies, Astrophys. J., 298, L7CrossRefGoogle Scholar
Kang, H., et al. 2005, Shock-Heated Gas in the Large-Scale Structure of the Universe, Astrophys. J., 620, 21CrossRefGoogle Scholar
Khare-Joshi, P. & Perry, J. J. 1982, Cosmological Implications of the Redshift Distribution of QSO Absorption Systems, MNRAS, 199, 785CrossRefGoogle Scholar
Kolb, E. W. & Turner, M. S. 1990, The Early Universe, Frontiers in Physics 69 (Boulder, CO: Westview Press)Google Scholar
Kronberg, P. P. 1994, Extragalactic Magnetic Fields, Rep. Prog. Phys., 57, 325CrossRefGoogle Scholar
Kronberg, P. P., Biermann, P. L., & Schwab, F. R. 1985, The Nucleus of M82 at Radio and X-Ray Bands – Discovery of a New Radio Population of Supernova Candidates, Astrophys. J., 291, 693CrossRefGoogle Scholar
Kronberg, P. P., Dyer, C. C., Burbidge, E. M., & Junkkarinen, V. T. A. 1991, Technique for Using Radio Jets as Extended Gravitational Lensing Probes, Astrophys. J., 367, L1CrossRefGoogle Scholar
Kronberg, P. P., Dyer, C. C., & Röser, H.-J. 1996, Estimates of the Global Masses of Two Distant Galaxies Using a New Type of Astrophysical Mass “Laboratory”, Astrophys. J., 472, 115CrossRefGoogle Scholar
Kronberg, P. P. & Perry, J. J. 1982, Absorption Lines, Faraday Rotation, and Magnetic Field Estimates for QSO Absorption-Line Clouds, Astrophys. J., 263, 518CrossRefGoogle Scholar
Kronberg, P. P., Perry, J. J., & Zukowski, E. L. H. 1990, The ‘Jet’ Rotation Measure Distribution and the Optical Absorption System Near the Z = 1.953 Quasar 3C 191, Astrophys. J. 355, L31CrossRefGoogle Scholar
Kronberg, P. P., Perry, J. J., & Zukowski, E. L. H. 1992, Discovery of Extended Faraday Rotation Compatible with Spiral Structure in an Intervening Galaxy at Z = 0.395 – New Observations of PKS 1229 – 021, Astrophys. J., 387, 528CrossRefGoogle Scholar
Kronberg, P. P., Reinhardt, M., & Simard-Normandin, M. 1977, On the Intergalactic Contribution to the Rotation Measures of QSO’s, Astron. Astrophys., 61, 771Google Scholar
Kronberg, P. P. & Simard-Normandin, M. 1976, New Evidence on the Origin of Rotation Measures in Extragalactic Radio Sources, Nature, 263, 653CrossRefGoogle Scholar
Kronberg, P. P. Unpublished.Google Scholar
Kulsrud, R. M. & Anderson, S. W. 1992, The Spectrum of Random Magnetic Fields in the Mean Field Dynamo Theory of the Galactic Magnetic Field, Astrophys. J., 396, 606CrossRefGoogle Scholar
Lavery, R. J., Seitzer, P., Suntzeff, N. B., Walker, A. R., & Da Costa, G. S. 1996, Distant Ring Galaxies as Evidence for a Steeply Increasing Galaxy Interaction Rate with Redshift Astrophys. J., 467, L1CrossRefGoogle Scholar
Medvedev, M. V. & Loeb, A. 1999, Generation of Magnetic Fields in the Relativistic Shock of Gamma-Ray Burst Sources, Astrophys. J., 526, 697CrossRefGoogle Scholar
Miniati, F. 2002, Intergalactic Shock Acceleration and the Cosmic Gamma-Ray Background, MNRAS, 337,199CrossRefGoogle Scholar
Nelson, A. H. 1973, On the Interpretation of Faraday Rotation Data, Pub. Ast. Soc. Japan, 25, 489Google Scholar
Oren, A. L. & Wolfe, A. M. 1995, A Faraday Rotation Search for Magnetic Fields in Quasar Damped Ly Alpha Absorption Systems, Astrophys. J., 445, 624CrossRefGoogle Scholar
Perry, J. J. & Dyson, J. E. 1990, 3 C 191 Revisited – Circumquasar Shells and Radio Jets, Astrophys. J., 361, 362CrossRefGoogle Scholar
Rees, M. J. & Reinhardt, M. 1972, Astron. Astrophys., 19, 104Google Scholar
Refsdal, S. 1964, The Gravitational Lens Effect, MNRAS, 128, 295CrossRefGoogle Scholar
Ryu, D., Kang, H., & Biermann, P. L. 1998, Cosmic Magnetic Fields in Large Scale Filaments and Sheets, Astrophys. J. 335, 19Google Scholar
Ryu, D., Kang, H., Cho, J., & Das, S. 2008, Turbulence and Magnetic Fields in the Large-Scale Structure of the Universe, Science, 320, 909CrossRefGoogle ScholarPubMed
Ryu, D., Schleicher, D. R. G., Treumann, R. A., Tsagas, C. G., & Widrow, L. M. 2012, Magnetic Fields in the Large-Scale Structure of the Universe, Space Sci. Rev., 166, 1Google Scholar
Schlickeiser, R. & Shukla, P. K. 2003, Cosmological Magnetic Field Generation by the Weibel Instability, Astrophys. J., 599, L57CrossRefGoogle Scholar
Schmidt, M. 1963, 3C 273: A Star-Like Object with Large Red-Shift, Nature, 197, 1040CrossRefGoogle Scholar
Springel, V. & Hernqvist, L. 2003, The History of Star Formation in a LCDM Universe, MNRAS, 339, 312CrossRefGoogle Scholar
Völk, H. J. 1989, The Correlation Between Radio and Far-Infrared Emission for Disk Galaxies – A Calorimeter Theory, Astron. Astrophys., 218, 67Google Scholar
Wallace, J. M. & Epperlein, E. M. 1991, Weibel Instability with Constant Driving Source, Phys. Fluids B Plasma Phys., 3, 1579CrossRefGoogle Scholar
Walsh, D., Carswell, R. F., & Weymann, R. J. 1979, 0957+561 A, B: Twin Quasistellar Objects or Gravitational Lens?, Nature, 279, 381CrossRefGoogle ScholarPubMed
Watson, A. M. & Perry, J. J. 1991, QSO Absorption Lines and Rotation Measures, MNRAS, 248, 58CrossRefGoogle Scholar
Weibel, E. 1959, Spontaneously Growing Transverse Waves in a Plasma Due to an Anisotropic Velocity Distribution, Phys. Rev. Lett., 2, 83CrossRefGoogle Scholar
Welter, G. L., Perry, J. J., & Kronberg, P. P. 1984, The Rotation Measure Distribution of QSOs and of Intervening Clouds - Magnetic Fields and Column Densities, Astrophys. J., 279, 19CrossRefGoogle Scholar
Whelan, Daniel J., Johnson, Jarrett L., Meiksin, Avery, Heger, Alexander, Even, Wesley, Fryer, Chris L. 2013, The Supernova that Destroyed a Protogalaxy: Prompt Chemical Enrichment and Supermassive Black Hole Growth, Astrophys. J., 774, 64CrossRefGoogle Scholar
Widrow, L. M. 2012, The First Magnetic Fields, Space Sci. Rev. 166, 37Google Scholar
Williams, R. E., Strittmatter, P. A., Carswell, R. F., & Craine, E. R. 1975, Splitting of Absorption Lines in 3C 191 Astrophys. J., 202, 296CrossRefGoogle Scholar
Willis, A. G. & Strom, R. G. 1978, Multifrequency Observations of Very Large Radio Galaxies. I - 3C 326, Astron. Astrophys., 62, 375Google Scholar
Wolfe, A. M., Lanzetta, K. M., Foltz, C. B., & Chaffee, F. H. 1995, The Large Bright QSO Survey for Damped Ly Alpha Absorption Systems, Astrophys. J., 454, 698CrossRefGoogle Scholar
Xu, Y., Kronberg, P. P., Habib, S., & Dufton, Q. W. 2006, A Faraday Rotation Search for Magnetic Fields in Large-scale Structure, Astrophys. J., 637, 19CrossRefGoogle Scholar
Yang, T.-Y. B., Arons, J., & Langdon, A. B. Evolution of the Weibel Instability in Relativistically Hot Electron-Positron Plasmas, Phys. Plas., 1, 3059CrossRefGoogle Scholar
Zwicky, F. 1937, Nebulae as Gravitational Lenses, Phys. Rev., 51, 290CrossRefGoogle Scholar

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×