Published June 1976
| Version v1
Journal article
PSR 1055-52 - a pulsar resembling the Crab Nebula pulsar
- 1. Tasmania Univ., Sandy Bay (Australia). Dept. of Physics
Description
Mean pulse profiles of the pulsar PSR 1055-52 have been measured at frequencies of 308, 400, 635 and 1400 MHz; in addition measurements have been made of the strong linear polarization at 1400 MHz. The pulse shape is found to be complex with a strong interpulse approximately midway between the main components. The average pulse from PSR 1055-52 displays certain remarkable similarities to that of the Crab Nebula pulsar PSR 0531 + 21. (author)
Additional details
Identifiers
Publishing Information
- Journal Title
- Monthly Notices of the Royal Astronomical Society
- Journal Volume
- 175
- Journal Issue
- 1
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 71P-75P
- ISSN
- 0035-8711
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 7269830
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CORRELATIONS; CRAB NEBULA; GHZ RANGE 01-100; MHZ RANGE 100-1000; POLARIZATION; PULSARS; RADIOWAVE RADIATION; VARIATIONS
- Descriptors DEC
- COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; FREQUENCY RANGE; GHZ RANGE; MHZ RANGE; NEBULAE; RADIATIONS; SUPERNOVA REMNANTS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent