Hostname: page-component-848d4c4894-cjp7w Total loading time: 0 Render date: 2024-06-17T18:49:26.353Z Has data issue: false hasContentIssue false

Neutral Hydrogen in the Bar of NGC 4151

Published online by Cambridge University Press:  12 April 2016

C. G. Mundell
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, U.K.
A. Pedlar
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, U.K.
D. L. Shone
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, U.K.
M. W. Asif
Affiliation:
Royal Greenwich Observatory, Madingly Rd., Cambridge CBS OEZ, UK
A. Robinson
Affiliation:
University of Cambridge, Institute of Astronomy, Madingly Road, Cambridge CB3 0HA, U.K.
D. J. Axon
Affiliation:
Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Bars are thought to play a crucial role in the fueling of AGN (see e.g., Mundell et al., in these proceedings and references therein), and as part of a project to investigate this, we have studied the neutral hydrogen structure in the bar of the Seyfert 1.5 galaxy NGC 4151.

High-sensitivity VLA observations have enabled us to image the neutral hydrogen emission from the bar of NGC 4151 in unprecedented detail, and is a continuation of the work by Pedlar et al. (1992).

Figure 1 shows images of integrated neutral hydrogen emission. The large scale emission extends over approximately 20 kpc and the outer part consists of a well-defined two-armed spiral which originates from a fat bar at a radius of about 5 kpc. The bar shows complex structure, including two sharp features which are reminiscent of the shocks seen in many simulations, e.g., Athanassoula (1992). These features appear to join the central 1-kpc ring discovered by Vila-Vilaró et al. (1994), and for which there appears a partial counterpart in neutral hydrogen emission.

Type
Posters for Part III and Part IV
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Athanassoula, E. 1992, MNRAS, 259, 345 Google Scholar
Mundell, C.G., Pedlar, A., Baum, S.A., O’Dea, C.P., Gallimore, J.F., & Brinks, E. 1995 MNRAS, 275, 67 Google Scholar
Pedlar, A., Howley, P., Axon., D.J. & Unger, S.W. 1992 MNRAS, 259, 369PGoogle Scholar
Vila-Vilaró, B., Robinson, A., Perez, E., Axon, D.J., Baum, S.A., G onzález-Delgado, R.M., Pedlar, A. et al. 1994, A&A, 302, 58VGoogle Scholar