Skip to main content

Thank you for visiting You are using a browser version with limited support for CSS. To obtain the best experience, we recommend you use a more up to date browser (or turn off compatibility mode in Internet Explorer). In the meantime, to ensure continued support, we are displaying the site without styles and JavaScript.

The Long Period Variations of UZ Persei


IN Harvard College Observatory Bulletin, No. 867, Feb. 1, 1929, there is a note by B. P. Gerasimovič on “UZ Persei, a Variable of Unusually Long Period”. The author found that the brightness of this variable star has two oscillations—short and long—with periods of about 90 and 907 days respectively. It is known that such oscillations are typical for μ Cephei.

This is a preview of subscription content, access via your institution

Access options

Rent or buy this article

Get just this article for as long as you need it


Prices may be subject to local taxes which are calculated during checkout

Author information

Authors and Affiliations


Rights and permissions

Reprints and Permissions

About this article

Cite this article

ZESSEWITSCH, W. The Long Period Variations of UZ Persei. Nature 124, 93–94 (1929).

Download citation

  • Issue Date:

  • DOI:


By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.


Quick links

Nature Briefing

Sign up for the Nature Briefing newsletter — what matters in science, free to your inbox daily.

Get the most important science stories of the day, free in your inbox. Sign up for Nature Briefing