Published November 15, 1972
| Version v1
Journal article
Pulse shape of the Crab Nebula pulsar Np 0532 as a function of color
Creators
Description
We find differences in the shape of the secondary pulse of NP 0532 in U, B, and V. The leading edge and peak are stronger at higher frequencies, relative to the trailing edge. The peak difference is about 3 percent between the U and the V.
Additional details
Identifiers
- DOI
- 10.1086/181074;
Publishing Information
- Journal Title
- The Astrophysical Journal
- Journal Volume
- 178
- Journal Issue
- 1
- Series
- Astrophys. J.
- Journal Page Range
- L13
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 4054973
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COLOR; CRAB NEBULA; PEAKS; PULSARS; PULSES; SHAPE
- Descriptors DEC
- CONFIGURATION; COSMIC RADIO SOURCES; NEBULAE; OPTICAL PROPERTIES; ORGANOLEPTIC PROPERTIES; PHYSICAL PROPERTIES; SUPERNOVA REMNANTS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent