On the mass of the X-ray binary cluster A399/A401

Details On the mass of the X-ray binary cluster A399/A401 On the mass of the X-ray binary cluster A399/A401

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.192..109k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 192, July 1980, p. 109-112.

Astronomy and Astrophysics

Astronomy

16

Galactic Clusters, Mass Distribution, Radial Velocity, X Ray Sources, Galactic Evolution, Velocity Measurement, X Ray Astronomy

Scientific paper

The mean radial velocity and the dispersion of velocities for the
cluster A399, component of the X-ray pair A399/A401, are determined from
nine galaxies. The difference in radial velocities of the clusters is
1000 km/s. The mass of the pair estimated in two ways lies within
3.3-9.9 x 10 to the 15th solar mass.

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