Nonradial pulsation in IOTA Herculis and 10 Lacertae /1975-1977/

Astronomy and Astrophysics – Astrophysics

Scientific paper

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B Stars, Early Stars, Periodic Variations, Variable Stars, Graphs (Charts), Pulse Amplitude, Pulse Duration, Radial Distribution, Radial Velocity, Stellar Models, Tables (Data), Traveling Waves, Wave Propagation

Scientific paper

Model line profiles are fitted to observations of two line-profile-variable B stars, Iota Her (B3 IV) and 10 Lac (O8 III), which straddle the Beta Cep strip. The periods observed in the two stars are confirmed; the lengths of the periods and the success in profile fitting suggest that the observed profile variations can only be identified with g-mode direct traveling waves. Both stars are shown to be complex nonradial pulsators capable of changing their amplitudes and periods on a time scale of months. The apparent documentation in Iota Her of a change from one mode to its harmonic in 2 to 3 days is discussed, and the observed variations in line strength are correlated with pulsational phase for strong lines of several ions. These variations are attributed to changes in a 'microturbulent' velocity. The results also indicate that stars of 7 to 8 solar masses may prefer to pulsate with basic periods of 10 to 14 hr, that 10 Lac may pulsate in a harmonic of a longer basic period, and that the inclinations of both Iota Her and 10 Lac appear to be large (sin i approximately equal to unity).

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