Skip to main content Accessibility help

We use cookies to distinguish you from other users and to provide you with a better experience on our websites. Close this message to accept cookies or find out how to manage your cookie settings.

Close cookie message
×
Hostname: page-component-848d4c4894-v5vhk Total loading time: 0 Render date: 2024-06-29T02:42:20.915Z Has data issue: false hasContentIssue false

6 - Magnetic field outflow from dwarf and starburst galaxies

Published online by Cambridge University Press:  22 September 2016

Philipp P. Kronberg
Philipp P. Kronberg
Affiliation:
University of Toronto
Get access

Summary

A summary is not available for this content so a preview has been provided. Please use the Get access link above for information on how to access this content.
Image of the first page of this content. For PDF version, please use the ‘Save PDF’ preceeding this image.'
Type
Chapter
Information
Cosmic Magnetic Fields , pp. 100 - 116
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

Alfvén, H. & Fälthammar, C.-G. 1963, Cosmical Electrodynamics (Oxford: Clarendon)Google Scholar
Beck, R., Loiseau, N., Hummel, E., Berkhuijsen, E. M., Grave, R., & Wielebinski, R. 1989, High-Resolution Polarization Observations of M31. I – Structure of the Magnetic Field in the Southwestern Arm, Astron. Astrophys., 222, 58Google Scholar
Beck, R. 2010, Galactic and Extragalactic Magnetic Fields, arXiv0810:2923v4 [astro-ph]Google Scholar
Bertone, S., Vogt, C., & Enßlin, T. E. 2006, Magnetic Field Seeding by Galactic Winds, MNRAS, 370, 319CrossRefGoogle Scholar
Birk, G. T., Wiechen, H., Lesch, H., & Kronberg, P. P. 2000, The Role of Kelvin-Helmholtz Modes in Superwinds of Primeval Galaxies for the Magnetization of the Intergalactic Medium, Astron. Astrophys., 353, 108Google Scholar
Carilli, C. L., Holdaway, M. A., Ho, P. T. P., & de Pree, C. G. 1992, Discovery of a Synchrotron-Emitting Halo Around NGC 253, Astrophys. J., 399, 59CrossRefGoogle Scholar
Chyży, K., Beck, R., Kohle, S., Klein, U., & Urbanik, M. 2000, Regular Magnetic Fields in the Dwarf Irregular Galaxy NGC 4449, Astron. Astrophys., 355, 128Google Scholar
Chyży, K. T., Soida, M., Bomans, D. J., Vollmer, B., Balkowski, Ch., Beck, R., & Urbanik, M. 2006, Large-Scale Magnetized Outflows from the Virgo Cluster Spiral NGC 4569: A Galactic Wind in a Ram Pressure Wind, Astron. Astrophys., 447, 465CrossRefGoogle Scholar
Clarke, D. A. 1993, 3-D MHD Simulations of Extragalactic Jets, in Jets in Extragalactic Radio Sources, ed. Röser, H. J. & Meisenheimer, K., Lecture Notes in Physics (Berlin: Springer-Verlag), 421, 243Google Scholar
Donnert, J., Dolag, K., Lesch, H., & Müller, E. 2009, Cluster Magnetic Fields from Galactic Outflows, MNRAS, 392, 1008CrossRefGoogle Scholar
Frank, A., Jones, T. W., Ryu, D., & Gaalaas, J. B. 1996, The Magnetohydrodynamic Kelvin-Helmholtz Instability: A Two-Dimensional Numerical Study, Astrophys. J., 460, 777CrossRefGoogle Scholar
Heckman, T. M., Armut, L., & Miley, G. K. 1990, On the Nature and Implications of Starburst-Driven Superwinds Astrophys. J. Suppl., 74, 833CrossRefGoogle Scholar
Kepley, A. A., Mühle, S., Everett, J., Zweibel, E. G., Wilcots, E. M., & Klein, U. 2010, The Role of the Magnetic Field in the Interstellar Medium of the Post-Starburst Dwarf Irregular Galaxy NGC 1569, Astrophys. J., 712, 536CrossRefGoogle Scholar
Krause, F. 1987, Dynamo Excitation in Very Large Scales, in Interstellar Magnetic Fields: Observation and Theory: Proceedings of a Workshop held at Schloss Ringberg, Tegernsee September 8–12, 1986, ed. Beck, R. & Gräve, R. (Berlin: Springer-Verlag), 8Google Scholar
Krause, M. 2009, Magnetic Fields and Star Formation in Spiral Galaxies, in Magnetic Fields in the Universe II: From Laboratory and Stars to the Primordial Universe, Cozumel, Mexico, January 28th to February 1st, 2008, ed. Esquivel, A. et al., Rev. Mex. Ast. Astrof., Ser. de Conf. (Mexico, D.F.: Instituto de Astronomia, Universidad Nacional Autonoma de Mexico), 36, 25Google Scholar
Kronberg, P. P. 1994, Extragalactic Magnetic Fields, Rep. Prog. Phys., 57, 325CrossRefGoogle Scholar
Kronberg, P. P., Biermann, P., & 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., Lesch, H., & Hopp, U. 1999, Magnetisation of the Intergalactic Medium by Primeval Galaxies, Astrophys. J., 511, 56CrossRefGoogle Scholar
Kronberg, P. P. & Wilkinson, P. N. 1975, High-Resolution, Multifrequency Radio Observations of M82, Astrophys. J., 200, 430CrossRefGoogle Scholar
Lesch, H., Crusius, A., Schlickeiser, R., & Wielebinski, R. 1989, Ring Currents and Poloidal Magnetic Fields in Nuclear Regions of Galaxies, Astron. Astrophys., 217, 99Google Scholar
Lo, K. Y., Cheung, K. W., Masson, C. R., Phillips, T. G., & Woody, D. P. 1985, Aperture synthesis observations of CO emission from M82, in ESO-IRAM-Onsala Workshop on (Sub)Millimeter Astronomy, Aspenas, Sweden, June 17–20, 1985, Proceedings (A86-39226 18–90), ed. Shaver, P.A. & Kjär, K., ESO Conf. Proc. (Garching: European Southern Observatory), 22, 197Google Scholar
Loiseau, N., Reuter, H.-P., Wielebinski, R., & Klein, U. 1988, A C-13O(2-1) Map of M82, Astron. Astrophys., 200, 1Google Scholar
McCarthy, P. J., van Breugel, W., & Heckman, T. 1987, Evidence for Large-Scale Winds from Starburst Galaxies. I – The Nature of the Ionized Gas in M82 and NGC 253, Astron. J., 93, 264CrossRefGoogle Scholar
Nakai, N., Hayashi, M., Handa, T., Sofue, Y., Hasagawa, T., & Sasaki, M. 1987, A Nuclear Molecular Ring and Gas Outflow in the Galaxy M82, Publ. Astr. Soc. Japan, 39, 685Google Scholar
Parker, E.N. 1976, Ring Currents and Poloidal Magnetic Fields in Nuclear Regions of Galaxies, Astron. Astrophys., 217, 99Google Scholar
Parker, E. N. 1979, Cosmical Magnetic Fields (Oxford: Clarendon)Google Scholar
Parker, E. N. 1992, Fast Dynamos, Cosmic Rays, and the Galactic Magnetic Field, Astrophys. J., 401, 137CrossRefGoogle Scholar
Reuter, H. P, Klein, U., Lesch, H., Wielebinski, R., & Kronberg, P. P. 1992, Gaps and Filaments in the Synchrotron Halo of M82 – Evidence for Poloidal Magnetic Fields, Astron. Astrophys., 256, 10Google Scholar
Reuter, H. P., Klein, U., Lesch, H., Wielebinski, R., & Kronberg, P. P. 1994, The Magnetic Field in the Halo of M 82. Polarized Radio Emission at Lambda-Lambda(6.2) and 3.6 CM, Astron. Astrophys., 282, 724Google Scholar
Ryu, D., Kang, H. S., & 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
Schaaf, R., Pietsch, W., Biermann, P. L., Kronberg, P. P., & Schmutzler, T. 1989, X-Ray Observation of the Starburst Galaxy M82, Astrophys. J., 336, 722CrossRefGoogle Scholar
Seaquist, E. R. & Odegard, N. 1991, A Nonthermal Radio Halo Surrounding M82, Astrophys. J., 369, 320CrossRefGoogle Scholar
Völk, H. J. & Atoyan, A. M. 2000, Early Starbursts and Magnetic Field Generation in Galaxy Clusters, Astrophys. J., 541, 88CrossRefGoogle Scholar
Weliachew, L., Fomalont, E. B., & Greisen, E. W. 1984, Radio Observations of H I and OH in the Center of the Galaxy M 82, Astron. Astrophys., 137, 335Google 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
×