Long term photometric monitoring with the Mercator telescope. Frequencies and mode identification of variable O-B stars

Peter de Cat (1) , Maryline Briquet (2) , Conny Aerts (3) , K. Goossens (2) , Sophie Saesen (2) , J. Cuypers (1) , K. Yakut (2) , Richard Scuflaire (4) , Marc-Antoine Dupret (5, 6) , K. Uytterhoeven (7) , H. van Winckel (2) , G. Raskin (2) , G. Davignon (2) , L. Le Guillou (2) , R. van Malderen (2) , M. Reyniers (2) , B. Acke (2) , W. de Meester (2) , J. Vanautgaerden (2) , Bart Vandenbussche (2) , Tijl Verhoelst (2) , Christoffel Waelkens (2) , Pieter Deroo (2) , K. Reyniers (2) , M. Ausseloos (2) , E. Broeders (2) , J. Daszynska-Daszkiewicz (2) , Jonas Debosscher (2) , S. de Ruyter (2) , K. Lefever (2) , G. Decin (2) , K. Kolenberg (2) , Anwesh Mazumdar (2) , C. van Kerckhoven (2) , Joris de Ridder (2) , Rachel Drummond (2) , Caroline Barban (2, 5, 6) , E. Vanhollebeke (2) , T. Maas (2) , Leen Decin (2)

1 Koninklijke Sterrenwacht van België
2 Instituut voor Sterrenkunde, Katholieke Universiteit Leuven
3 Instituut voor Sterrenkunde, K.U. Leuven, Celestijnenlaan 200 B, 3001 Leuven, Belgium Department of Astrophysics, Radboud University Nijmegen
4 Institut d'Astrophysique, Géophysique et Océanographie, Université de Liège
5 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique
6 Pôle Astronomie du LESIA
7 Instituut voor Sterrenkunde, K.U. Leuven, Celestijnenlaan 200 B, 3001 Leuven, Belgium INAF - Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate, Italy mercator Telescope

Aims: We selected a large sample of O-B stars that were considered as (candidate) slowly pulsating B, beta Cep, and Maia stars after the analysis of their hipparcos data. We analysed our new seven passband geneva data collected for these stars during the first three years of scientific operations of the mercator telescope. We performed a frequency analysis for 28 targets with more than 50 high-quality measurements to improve their variability classification. For the pulsating stars, we tried both to identify the modes and to search for rotationally split modes. <BR />Methods: We searched for frequencies in all the geneva passbands and colours by using two independent frequency analysis methods and we applied a 3.6 S/N-level criterion to locate the significant peaks in the periodograms. The modes were identified by applying the method of photometric amplitudes for which we calculated a large, homogeneous grid of equilibrium models to perform a pulsational stability analysis. When both the radius and the projected rotational velocity of an object are known, we determined a lower limit for the rotation frequency to estimate the expected frequency spacings in rotationally split pulsation modes. <BR />Results: We detected 61 frequencies, among which 33 are new. We classified 21 objects as pulsating variables (7 new confirmed pulsating stars, including 2 hybrid beta Cep/SPB stars), 6 as non-pulsating variables (binaries or spotted stars), and 1 as photometrically constant. All the Maia candidates were reclassified into other variability classes. We performed mode identification for the pulsating variables for the first time. The most probable l value is 0, 1, 2, and 4 for 1, 31, 9, and 5 modes, respectively, including only 4 unambiguous identifications. For 7 stars we cannot rule out that some of the observed frequencies belong to the same rotationally split mode. For 4 targets we may begin to resolve close frequency multiplets.

Domaines: Astrophysique [astro-ph]

Peter de Cat, Maryline Briquet, Conny Aerts, K. Goossens, Sophie Saesen, et al.. Long term photometric monitoring with the Mercator telescope. Frequencies and mode identification of variable O-B stars. Astronomy and Astrophysics - A&A, 2007, 463, pp.243-249. ⟨10.1051/0004-6361:20066202⟩. ⟨hal-03786207⟩