Absence of Pulsar Characteristics in Several X-ray Sources
- 1 January 1969
- journal article
- letter
- Published by Springer Nature in Nature
- Vol. 221 (5178) , 345-347
- https://doi.org/10.1038/221345a0
Abstract
No abstract availableKeywords
This publication has 20 references indexed in Scilit:
- Rapid Changes in the Optical Intensity and Radial Velocities of the X-Ray Source SCO X-1The Astrophysical Journal, 1968
- Soft X-Rays from Scorpius XR-1The Astrophysical Journal, 1968
- Positions of Four PulsarsNature, 1968
- Possible Detection of a Dense Intergalactic PlasmaThe Astrophysical Journal, 1968
- Pulsation Periods of Rotating White DwarfsNature, 1968
- Heating of H i Regions by Energetic ParticlesThe Astrophysical Journal, 1968
- Far Ultra-violet Spectra of Orion StarsNature, 1967
- Ultrashort-Period Stellar Oscillations. I. Results from White Dwarfs, Old Novae, Central Stars of Planetary Nebulae, 3c 273, and Scorpius XR-1The Astrophysical Journal, 1967
- On the Nature of the Source of X-Ray Emission of SCO XR-1.The Astrophysical Journal, 1967
- On a Possible Interstellar Galactic Corona.The Astrophysical Journal, 1956