Magnetic Bp and Ap stars in the H-R diagram

被引：0

作者：

Hubrig, S ^{[1
]}

North, P ^{[1
]}

Mathys, G ^{[1
]}

机构：

[1] Univ Potsdam, D-14469 Potsdam, Germany

来源：

PROCEEDINGS OF THE 26TH MEETING AND WORKSHOP OF THE EUROPEAN WORKING GROUP ON CP STARS | 1998年 / 27卷 / 03期

关键词：

H-R diagram; magnetic stars;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The positions in the H-R diagram of strongly magnetic Ap and Bp stars are compared with those of normal main sequence-stars of types B7 to F2, with a view to investigating possible differences in evolutionary status between magnetic and non-magnetic stars. The normal B7-F2 stars fill the whole width of the main sequence band with some concentration towards the ZAMS, whereas the magnetic stars are only rarely found close to either the zero-age or terminal-age sequences.

引用

页码：249 / 251

页数：3

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