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- W1978786007 abstract "Context. HD 181231 and HD 175869 are two late rapidly rotating Be stars, which have been observed using high-precision photometry with the CoRoT satellite during about five consecutive months and 27 consecutive days, respectively. An analysis of their light curves, by Neiner and collaborators and Gutiérrez-Soto and collaborators respectively, showed that several independent pulsation g-modes are present in these stars. Fundamental parameters have also been determined by these authors using spectroscopy." @default.
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- W1978786007 date "2012-02-28" @default.
- W1978786007 modified "2023-09-30" @default.
- W1978786007 title "Seismic modelling of the late Be stars HD 181231 and HD 175869 observed with CoRoT: a laboratory for mixing processes" @default.
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- W1978786007 doi "https://doi.org/10.1051/0004-6361/201118151" @default.
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