Abstract
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
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Rent or buy this article
Get just this article for as long as you need it
$39.95
Prices may be subject to local taxes which are calculated during checkout
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
ZESSEWITSCH, W. The Long Period Variations of UZ Persei. Nature 124, 93–94 (1929). https://doi.org/10.1038/124093c0
Issue Date:
DOI: https://doi.org/10.1038/124093c0
Comments
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.
