Published November 4, 1987
| Version v1
Journal article
Two types of pulsar
Description
Some arguments for the subdivision of pulsars into two classes are considered: (i) short-period pulsars described by Smith's (1973) model and (ii) long-period pulsars for which the hollow-cone model is valid. The data for PSR 1937 + 21 (P = 1.56 ms) are in good agreement with this conception, this pulsar being a typical representative of the first group of pulsars
Additional details
Publishing Information
- Journal Title
- Australian Journal of Physics
- Journal Volume
- 40
- Journal Issue
- 6
- Series
- Aust. J. Phys.
- Journal Page Range
- 731-739
- ISSN
- 0004-9506
- CODEN
- AUJPA
Conference
- Title
- Joint USSR-Australia Shklovskii symposium on supernova remnants and pulsars.
- Dates
- 8-11 Jun 1986.
- Place
- Pushchino (USSR).
INIS
- Country of Publication
- Australia
- Country of Input or Organization
- Australia
- INIS RN
- 20043390
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- MATHEMATICAL MODELS; PULSARS; RADIOWAVE RADIATION
- Descriptors DEC
- COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; RADIATIONS