From Wikipedia, the free encyclopedia
||This article may be expanded with text translated from the corresponding article in the Italian Wikipedia. (August 2013)|
49 Ceti was identified as “Vega-like” debris-disk hosting A star based on infrared emission detected by the IRAS satellite.
49 Ceti has been identified as a member of the 40-Myr old Argus Association .
- Sadakane, K. & Nishida, M. 1986, Publ. Astron. Soc. Pacific, Vol. 98, p. 685.
- Zuckerman, B. & Song, I. 2012 arXiv:1207.1747
|This main-sequence-star-related article is a stub. You can help Wikipedia by expanding it.|