Abstract
It is shown that the magnetic measurements of HD 133029 exhibit a correlation of magnetic intensity with exposure length. Due to this effect a re-examination of the star's period was undertaken, resulting in a new period of 0.168 days. The significance of such a short period is discussed. It is argued that this short variation cannot be due to an oblique rotator.
Original language | English |
---|---|
Pages (from-to) | 322-329 |
Number of pages | 8 |
Journal | Astrophysics and Space Science |
Volume | 11 |
Issue number | 2 |
DOIs | |
State | Published - 1 May 1971 |
Externally published | Yes |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science