Science, Том 291John Michels (Journalist) American Association for the Advancement of Science, 2001 |
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Стр. 94
... stars and ( B ) variable stars only . The data shown correspond to one epoch ( reference scan ) . The solid line indicates the ZAMS at the assumed distance of 460 pc . The arrow indicates the shift of a star's position in the diagram ...
... stars and ( B ) variable stars only . The data shown correspond to one epoch ( reference scan ) . The solid line indicates the ZAMS at the assumed distance of 460 pc . The arrow indicates the shift of a star's position in the diagram ...
Стр. 95
... stars in la are older than stars in OB1b . Stars in OB1b seem to fall between the isochrones corresponding to 1 to 3 Ma , whereas stars in OB1a seem to fall between 3 and 30 Ma , in agreement with photometric age estimates for the high- ...
... stars in la are older than stars in OB1b . Stars in OB1b seem to fall between the isochrones corresponding to 1 to 3 Ma , whereas stars in OB1a seem to fall between 3 and 30 Ma , in agreement with photometric age estimates for the high- ...
Стр. 96
... stars of O , B , and A spectral types in OB1a ( blue open triangles ) and in OB1b ( red open triangles ) . The position of the belt stars ( large star symbols ) and the limits of the scan ( dotted lines ) are indicated as reference ...
... stars of O , B , and A spectral types in OB1a ( blue open triangles ) and in OB1b ( red open triangles ) . The position of the belt stars ( large star symbols ) and the limits of the scan ( dotted lines ) are indicated as reference ...
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