Long-term photometric monitoring with the Mercator telescope***

Authors :: Cuypers, J.
Aerts, C.
De Cat, P.
De Ridder, J.
Goossens, K.
Schoenaers, C.
Uytterhoeven, K.
Acke, B.
Davignon, G.
Debosscher, J.
Decin, L.
De Meester, W.
Deroo, P.
Drummond, R.
Kolenberg, K.
Lefever, K.
Raskin, G.
Reyniers, M.
Saesen, S.
Vandenbussche, B.
Van Malderen, R.
Verhoelst, T.
Van Winckel, H.
Waelkens, C.
Cuypers, J.
Aerts, C.
De Cat, P.
De Ridder, J.
Goossens, K.
Schoenaers, C.
Uytterhoeven, K.
Acke, B.
Davignon, G.
Debosscher, J.
Decin, L.
De Meester, W.
Deroo, P.
Drummond, R.
Kolenberg, K.
Lefever, K.
Raskin, G.
Reyniers, M.
Saesen, S.
Vandenbussche, B.
Van Malderen, R.
Verhoelst, T.
Van Winckel, H.
Waelkens, C.
Source :: Astronomy and Astrophysics; June 2009, Vol. 499 Issue: 3 p967-982, 16p
Publication Year :: 2009
Abstract: Context. γDor stars are excellent targets for asteroseismology since the gravity modes present in these stars probe the deep stellar interiors. Mode identification will improve the knowledge of these stars considerably.

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