Observations of a new transition in the emission from CYG X-1

Details Observations of a new transition in the emission from CYG X-1 Observations of a new transition in the emission from CYG X-1

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.256..108h&link_type=abstract

Nature, vol. 256, July 10, 1975, p. 108, 109. Research supported by the University of Maryland.

Astronomy and Astrophysics

Astronomy

20

Radiant Flux Density, Spaceborne Astronomy, Stellar Radiation, Variable Stars, X Ray Astronomy, X Ray Stars, Ariel Satellites, Satellite Observation, Spectral Resolution

Scientific paper

Data from the all-sky X-ray monitor aboard Ariel V were used to establish that a sudden transition had occurred in emissions from Cyg X-1 on April 22, 1975. Cyg X-1 has been observed almost continuously since around November 1, 1974, and has been relatively constant in apparent magnitude until the reported effect. The results of these observations are discussed.

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