arXiv:1311.2818 [astro-ph.SR]AbstractReferencesReviewsResources
Interpretation of the oscillation spectrum of HD 50230 - a failure of richness
Wojciech Szewczuk, Jadwiga Daszyńska-Daszkiewicz, Wojciech Dziembowski
Published 2013-11-12Version 1
Attempts to interpret the observed oscillation spectrum of the SPB star HD 50230 are reported. We argue that a nearly equidistant period spacing found in the oscillation spectrum of the star is most likely accidental. The observed period distribution requires excitation of modes with the degree $\ell>4$. Much more may be learned from the rich oscillation spectrum of the star but most of the work is still ahead of us.
Comments: Proceedings IAU Symposium No. 301
Categories: astro-ph.SR
Related articles: Most relevant | Search more
arXiv:2208.05488 [astro-ph.SR] (Published 2022-08-10)
Magnetic braking saturates: evidence from the period distribution of low-mass eclipsing binaries from ZTF
Kareem El-Badry, Charlie Conroy, Jim Fuller, Rocio Kiman, Jan van Roestel, Antonio C. Rodriguez, Kevin B. Burdge
arXiv:1106.4931 [astro-ph.SR] (Published 2011-06-24)
On the period distribution of cluster RR Lyrae stars to constrain their helium content: the case of omega Centauri
Marcella Marconi, Giuseppe Bono, Filippina Caputo, Anna M. Piersimoni, Adriano Pietrinferni, Robert F. Stellingwerf
arXiv:1203.4577 [astro-ph.SR] (Published 2012-03-20)
Chromospheric magnetic fields. Observations, simulations and their interpretation