2017
DOI: 10.1017/s1743921317008274 View full text |Buy / Rent full text
|
|

Abstract: Recent studies of interstellar scattering frequency evolution indicate, that for a large number of pulsars the measured scatter time to frequency scaling does not follow predictions based upon simple scattering models. The number of such deviations suggests, that what was previously known as “anomalous scattering” is actually quite normal for a large subset of the pulsar population. New observations are needed, especially at low frequencies, to study the scattering of low-DM objects. In this regard even small … Show more

Help me understand this page

Search citation statements

Order By: Relevance
0
0
0
0
0
0
0
0

Publication Types

Select...

Relationship

0
0

Authors

Journals