Published June 1982
| Version v1
Journal article
On the implications of the radio and X-ray pulsar in the supernova remnant MSH 15-52
- 1. Raman Research Inst., Bangalore (India)
Description
Comparison of the X-ray nebulosity surrounding the X-ray and radio pulsar in the shell-type SNR MSH 15-52 with the Crab nebula leads to an initial period for the pulsar approximately 70 ms. The association of the pulsar with the shell remnant confirms the validity of the calibrators. (author)
Additional details
Publishing Information
- Journal Title
- Curr. Sci.
- Journal Volume
- 51
- Journal Issue
- 12
- Series
- Curr. Sci.
- Journal Page Range
- 596-599
- ISSN
- 0011-3891
- CODEN
- CUSCA
INIS
- Country of Publication
- India
- Country of Input or Organization
- India
- INIS RN
- 17020565
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- AGE ESTIMATION; PULSARS; RADIOWAVE RADIATION; SUPERNOVA REMNANTS; X RADIATION
- Descriptors DEC
- COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; RADIATIONS
Optional Information
- Notes
- 16 refs.