Royal Observatory Bulletins

Royal Observatory Bulletins

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This is also true in the Jfv, t (Hertzsprung-Russell) diagram. The significance of this departure is not clear, for it is always possible for a star to simulate the proper motion of the Hyades without any physical for even kinematical) connection. 7. ... Eggen and Sandage (1959) tentatively suggest that HD 84937, -3Ad 2525 and two other stars form a moving group with (UtV, W ... (U, V, W = +106, -150, +8). 24.

Title:Royal Observatory Bulletins
Author:Royal Greenwich Observatory
Publisher: - 1966


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