NASA NTRS · 19750051493
Rocket observations of the Perseus X-ray source
Abstract
The spectrum and angular distribution of soft X-ray emission from the source in the Perseus cluster has been observed. A prominent feature of this source is a point-like component at the position of NGC 1275. Preliminary analysis indicates that the spectrum of this source does not rise as steeply at energies below 1 keV as has been reported previously.
Keep this discovery
Explore connections, maps & timelines
Catura, R. C., Acton, L. W.. 1975-01-01. Rocket observations of the Perseus X-ray source. https://ntrs.nasa.gov/citations/19750051493
Cite the original work for its findings. Save a collection to share your selection of sources.