The X-ray source in NGC 1851

Details The X-ray source in NGC 1851 The X-ray source in NGC 1851

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....59l..23b&link_type=abstract

Astronomy and Astrophysics, vol. 59, no. 2, July 1977, p. L23-L26.

Astronomy and Astrophysics

Astrophysics

7

Globular Clusters, Periodic Variations, Radial Velocity, Stellar Evolution, X Ray Sources, Astronomical Photometry, Emission Spectra, H Beta Line, X Ray Spectra, X Ray Stars

Scientific paper

Measurements of the radial velocity of the highly evolved star UV5 in
the globular cluster NGC 1851 indicate that it is variable with a 15-day
period. Photometrically, the star does not appear to vary, but H-beta
occasionally shows an emission component. On the basis of these
characteristics, UV5 is put forward as the X-ray source in NGC 1851.

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