SIMBAD references

1999PASP..111..840K - Publ. Astron. Soc. Pac., 111, 840-844 (1999/July-0)

γ Doradus stars: defining a new class of pulsating variables.

KAYE A.B., HANDLER G., KRISCIUNAS K., PORETTI E. and ZERBI F.M.

Abstract (from CDS):

In this paper we describe a new class of pulsating stars, the prototype of which is the bright, early, F-type dwarf γ Doradus. These stars typically have between 1 and 5 periods ranging from 0.4 to 3 days with photometric amplitudes up to 0.1 mag in Johnson V. The mechanism for these observed variations is high-order, low-degree, nonradial, gravity-mode pulsation.

Abstract Copyright: ∼

Journal keyword(s): Stars: Oscillations - Stars: Variables: Other

Simbad objects: 14

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