4.7 Article

PSR B1133+16: radio emission height and plasma composition

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 435, Issue 1, Pages L11-L13

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnrasl/slt083

Keywords

instabilities; plasmas; pulsars: general; stars: neutron

Ask authors/readers for more resources

Recent operation of LOFAR by Hassall et al. has produced severe constraints on the size and altitude of the 40 MHz emission region in this pulsar. It is shown that these limits, given a limited number of unexceptionable assumptions, demonstrate that an electron-positron plasma cannot be the source of the emission. A physically acceptable plasma source composed of protons and ions arises naturally in pulsars having positive corotational polar-cap charge density. Acceptance of this would greatly clarify the classification of pulsar types within the whole.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.7
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available