Published 1978
| Version v1
Book
An interpretation of the phenomenon of drifting subpulses from pulsars
Creators
- 1. Nagoya Univ. (Japan). Dept. of Physics
- 2. Scuola Normale Superiore, Pisa (Italy)
Description
One of the most remarkable features of pulsed signals from pulsars is the complex pattern of phase modulation, which results in a systematic drift of successive subpulses across the average pulse window centred on the expected time of arrival of the pulse. It is suggested that this phenomenon might be explained in terms of a model of neutron star spot for pulsars. (C.F.)
Additional details
Publishing Information
- Publisher
- North-Holland.
- Imprint Place
- Amsterdam, Netherlands
- ISBN
- 0-7204-0720-3
- Imprint Title
- Physics and astrophysics of neutron stars and black holes
- Journal Page Range
- p. 771-773.
Conference
- Title
- International School of Physics 'Enrico Fermi' on physics and astrophysics of neutron stars and black holes.
- Dates
- 14 - 26 Jul 1975.
- Place
- Varenna, Italy.
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 10475265
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- COSMIC GASES; EMISSION; NEUTRON STARS; PULSARS; PULSES; RADIOWAVE RADIATION; ROTATION; STAR MODELS
- Descriptors DEC
- COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; FLUIDS; GASES; MATHEMATICAL MODELS; RADIATIONS; STARS