Book contents
- Frontmatter
- Contents
- Preface
- Part I Discoveries and Techniques
- Part II Observed Physical Characteristics
- 8 Pulse Profiles
- 9 The Variability of Pulsar Emission
- 10 Millisecond Pulsars
- 11 Magnetars
- 12 Thermal X-rays from Neutron Stars
- Part III Neutron Star Physics
- Part IV Environments and the Interstellar Medium
- References
- Index
8 - Pulse Profiles
from Part II - Observed Physical Characteristics
Published online by Cambridge University Press: 21 July 2022
- Frontmatter
- Contents
- Preface
- Part I Discoveries and Techniques
- Part II Observed Physical Characteristics
- 8 Pulse Profiles
- 9 The Variability of Pulsar Emission
- 10 Millisecond Pulsars
- 11 Magnetars
- 12 Thermal X-rays from Neutron Stars
- Part III Neutron Star Physics
- Part IV Environments and the Interstellar Medium
- References
- Index
Summary
Most of our understanding of the location and nature of the beamed emission comes from the pulse profiles, which are available over the whole electromagnetic spectrum. The radio profiles are the most detailed, with observations of polarisation, width and components.
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- Information
- Pulsar Astronomy , pp. 121 - 138Publisher: Cambridge University PressPrint publication year: 2022