g-modes in the late-type Be star β CMi detected by the MOST satellite^1

Details g-modes in the late-type Be star β CMi detected by the MOST satellite^1 g-modes in the late-type Be star β CMi detected by the MOST satellite^1

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007coast.150..215s&link_type=abstract

Communications in Astroseismology, Vol. 150, p.215

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The Microvariability and Oscillations of Stars (MOST) satellite has detected low-amplitude light variations (Δ m˜1 mmag) in the late-type Be star β CMi (B8Ve). The photometric variations have periods of ˜ 0.3 days. This is consistent with high-order, prograde (m = -1) g modes %excited by the Fe-bump of opacity at T˜ 2× 10^5K of a nearly critically rotating 3.5 M_&sun; model.

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