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Magnetic Field of a Spiral Galaxy

Jul 21 2020

VLA radio data from Yelena Stein and Ralf-Juergen Dettmar (Ruhr University Bochum). The observations are part of the project Continuum HAlos in Nearby Galaxies -- an EVLA Survey (CHANG-ES) led by Judith Irwin (Queen’s University, Canada). The optical data are from the Sloan Digital Sky Survey (www.sdss.org). The ionized hydrogen data (red) are from the 0.9m telescope of the Kitt Peak National Observatory, collected by Richard J. Rand of the University of New Mexico. The software code for tracing the magnetic field lines was adapted by Y. Stein from the Linear Integral Convolution code provided by Arpad Miskolczi of Ruhr University Bochum.

If you imagined a galaxy like the milky way, would you think of galaxy-wide magnetic fields? Probably not. The presented image of the galaxy NGC 4217 tells us that we should.

This image shows the huge extent of a spiral galaxy's magnetic field. The galaxy NGC 4217 is a star-forming, spiral galaxy, similar to our own Milky Way, 67 million light-years from Earth in the constellation Ursa Major. The galaxy is seen edge-on in a visible-light image from the Sloan Digital Sky Survey and Kitt Peak National Observatory, and the magnetic field lines, shown as green, are revealed by the National Science Foundation's Karl G. Jansky Very Large Array (VLA) radio telescope.

The magnetic field lines extend as much as 22,500 light-years beyond the galaxy's disk. Scientists know that magnetic fields play an important role in many processes, such as star formation, within galaxies. However, it is not fully understood how such huge magnetic fields are generated and maintained. A leading explanation, called the dynamo theory, suggests that magnetic fields are generated by the motion of plasma within the galaxy's disk. Ideas about the cause of the kinds of large vertical extensions seen in this image are more speculative, and astronomers hope that further observations and more analysis will answer some of the outstanding questions.

Yelena Stein and collaborators around the world show their results in the scientific paper "CHANG-ES XXI. Transport processes and the X-shaped magnetic field of NGC 4217: off-center superbubble structure" (DOI: https://www.aanda.org/10.1051/0004-6361/202037675).

In this paper, the enormous galaxy-wide magnetic field of NGC 4217 is revealed, shown in the image. Further analysis on the magnetic field revealed a helix-like magnetic field in the extension to the north. NGC 4217 shows loop and outflow structures throughout the galaxy observed in radio continuum emission and optical wavelengths, probably induced by stellar winds and/or the combined action of several supernova explosions.


Crédits:
Composite image by Yelena Stein of the Centre de Données astronomiques de Strasbourg (CDS) with the support of Jayanne English (University of Manitoba).

VLA radio data from Yelena Stein and Ralf-Juergen Dettmar (Ruhr University Bochum). The observations are part of the project Continuum HAlos in Nearby Galaxies -- an EVLA Survey (CHANG-ES) led by Judith Irwin (Queen’s University, Canada). The optical data are from the Sloan Digital Sky Survey (www.sdss.org). The ionized hydrogen data (red) are from the 0.9m telescope of the Kitt Peak National Observatory, collected by Richard J. Rand of the University of New Mexico. The software code for tracing the magnetic field lines was adapted by Y. Stein from the Linear Integral Convolution code provided by Arpad Miskolczi of Ruhr University Bochum.

The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.


Article: Stein Y. et al., 2020, A&A, "CHANG-ES XXI. Transport processes and the X-shaped magnetic field of NGC 4217: off-center superbubble structure"

Contact: Yelena Stein (Observatoire astronomique de Strasbourg) yelena.stein@astro.unistra.fr

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