Locating the intense interstellar scattering towards the inner Galaxy

Locating the intense interstellar scattering towards the inner Galaxy

We use VLBA+VLA observations to measure the sizes of the scatter-broadened images of six of the most heavily scattered known pulsars: three within the Galactic Centre (GC) and three elsewhere in the inner Galactic plane (Delta l < 20 degrees). By combining the measured sizes with temporal pulse b...

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Bibliographic Details
Main Authors: Dexter, J., Deller, A., Bower, G. C., Demorest, P., Kramer, M., Stappers, B.W., Lyne, A. G., Kerr, M., Spitler, L. G., Psaltis, D., Johnson, M., Narayan, R.
Other Authors: Univ Arizona
Language:en
Published: OXFORD UNIV PRESS 2017
Subjects:
scattering
pulsars: general
H II regions
ISM: supernova remnants
Galaxy: centre
Online Access:http://hdl.handle.net/10150/625730
http://arizona.openrepository.com/arizona/handle/10150/625730

Internet

http://hdl.handle.net/10150/625730
http://arizona.openrepository.com/arizona/handle/10150/625730

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