Mu Ceti is an A9
giant star. It has been suspected to be a
δ Scuti variable,[4] but most studies find it to be of constant brightness.[8][9]
Three companions were all discovered during
occultations of Mu Ceti by the
Moon. An orbit was derived for the brightest with a period of 1,202 days.[6] Later studies have failed to find any evidence of these companions.[10]
^Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1.
Bibcode:
2009yCat....102025S.
^Gray, R. O; Corbally, C. J; Garrison, R. F; McFadden, M. T; Robinson, P. E (2003). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I". The Astronomical Journal. 126 (4): 2048.
arXiv:astro-ph/0308182.
Bibcode:
2003AJ....126.2048G.
doi:
10.1086/378365.
S2CID119417105.
^
abHauck, B (1971). "Short period variable stars. V. Delta Scuti-type stars in the Geneva system". Astronomy and Astrophysics. 11: 79.
Bibcode:
1971A&A....11...79H.
^Breger, Michel (1969). "Short-Period Variability of b, a, and F Stars. III. A Survey of Delta Scuti Variable Stars". Astrophysical Journal Supplement. 19: 79.
Bibcode:
1969ApJS...19...79B.
doi:
10.1086/190199.