Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-03-29
published in ApJ 570, L17-L20 (2002)
Astronomy and Astrophysics
Astrophysics
minor changes
Scientific paper
10.1086/340931
Pulsars provide unique probes of the large-scale interstellar magnetic field in the Galactic disk. Up to now, the limited Galactic distribution of the known pulsar population has restricted these investigations to within a few kiloparsec of the Sun. The Parkes multibeam pulsar survey has discovered many more-distant pulsars which enables us for the first time to explore the magnetic field in most of the nearby half of the Galactic disk. Here we report the detection of counterclockwise magnetic fields in the Norma spiral arm using pulsar rotation measures. The fields are coherent in direction over a linear scale of $\sim 5$ kpc along the arm and have a strength of $-4.4\pm0.9$ $\mu$G. The magnetic field between the Carina-Sagittarius and Crux-Scutum arms is confirmed to be coherent from $l\sim45\degr$ to $l\sim305\degr$ over a length of $\sim 10$ kpc. These results strengthen arguments for a bisymmetric spiral model for the field configuration in the Galactic disk.
Han Jian-Long
Lyne Andrew G.
Manchester Richard N.
Qiao Guo Jun
No associations
LandOfFree
Counterclockwise magnetic fields in the Norma spiral arm does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Counterclockwise magnetic fields in the Norma spiral arm, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Counterclockwise magnetic fields in the Norma spiral arm will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-240714