Article (Scientific journals)
The field high-amplitude SX Phoenicis variable BL Camelopardalis: results from a multisite photometric campaign. I. Pulsation
Rodríguez, E.; Fauvaud, S.; Farrell, J. A. et al.
2007In Astronomy and Astrophysics, 471, p. 255-264
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Keywords :
stars: variables: delta Sct; stars: individual: BL Camelopardalis; stars: oscillations; techniques: photometric
Abstract :
[en] Context: BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very complex frequency spectrum is detected, with a number of independent nonradial modes excited, unusual among the high-amplitude pulsators in the Lower Classical Instability Strip. Aims: An extensive and detailed study has been carried out to investigate the pulsational content and properties of this object. Methods: The analysis is based on 283 h of CCD observations obtained in the Johnson V filter, during a long multisite photometric campaign carried out along the Northern autumn-winter of 2005-2006. Additionally, multicolour BI photometry was also collected to study the phase shifts and amplitude ratios, between light curves obtained in different filters, for modal discrimination of the main excited modes. Results: The detailed frequency analysis revealed a very rich and dense pulsational content consisting of 25 significant peaks, 22 of them corresponding to independent modes: one is the already known main periodicity f[SUB]0[/SUB] = 25.5765 cd[SUP]-1[/SUP] (Delta V = 153 mmag) and the other 21 are excited modes showing very small amplitudes. Some additional periodicities are probably still remaining in the residuals. This represents the most complex spectrum ever detected in a high-amplitude pulsator of this type. The majority of the secondary modes suspected from earlier works are confirmed here and, additionally, a large number of new peaks are detected. The amplitude of the main periodicity f[SUB]0[/SUB] seems to be stable during decades, but the majority of the secondary modes show strong amplitude changes from one epoch to another. The suspected fundamental radial nature of the main periodicity of BL Cam is confirmed, while the secondary peak f[SUB]1[/SUB] = 25.2523 cd[SUP]-1[/SUP] is identified as a nonradial mixed mode g[SUB]4[/SUB] with l = 1. The radial double-mode nature, claimed by some authors for the main two frequencies of BL Cam, is not confirmed. Nevertheless, the frequency f[SUB]6[/SUB] = 32.6464 cd[SUP]-1[/SUP] could correspond to the first radial overtone.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Rodríguez, E.;  Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain
Fauvaud, S.;  Association AstroQueyras, Le Bois de Bardon, Taponnat, 16110 La Rochefoucauld, France ; Groupe Européen d'Observations Stellaires (GEOS), 23 Parc de Levesville, 28300 Bailleau l'Evêque, France
Farrell, J. A.;  Sulphur Flats Observatory, 449 Sulphur Creek Road, Jemez Springs, NM 87025, USA
Zhou, A*-Y;  National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 China
Sareyan, J*-P;  Observatoire de la Côte d'Azur, BP 4229, 06304 Nice cedex 4, France
López-González, M. J.;  Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain
Dupret, Marc-Antoine ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique
Grigahcéne, A.;  CRAAG, Algiers Observatory, BP 63 Bouzareah 16340, Algiers, Algeria
De Ridder, J.;  Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium
Klingenberg, G.;  Variable Star Section, Norwegian Astronomical Society, PO Box 1029 Blindern, 0315 Oslo, Norway
Wolf, M.;  Astronomical Institute, Charles University Prague, V Holesovickach 2, 180 00 Praha 8, Czech Republic
van Cauteren, P.;  Beersel Hills Observatory, B-Beersel, Belgium
Lampens, P.;  Koninklijke Sterrenwacht van België, Ringlaan 3, 1180 Brussel, Belgium
Martínez, D.;  Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain
Casanova, V. M.;  Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain
Aceituno, F. J.;  Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain
Helvaci, M.;  Ankara University, Science Faculty, Department of Astronomy and Space Sciences, 06100 Ankara, Turkey
Hintz, E. G.;  Department of Physics and Astronomy, Brigham Young University, N283 ESC, Provo, UT 84602, USA
Král, L.;  Observatory and Planetarium of Johann Palisa, VSB-Technical University, Listopadu 15, 708 33 Ostrava-Poruba, Czech Republic
Fumagalli, F.;  Groupe Européen d'Observations Stellaires (GEOS), 23 Parc de Levesville, 28300 Bailleau l'Evêque, France
Simonetti, J. H.;  Martin Observatory, Physics Dep., Virginia Polytechnic Institute & State Univ., Blacksburg, VA 24061, USA
Granslo, B. H.;  Variable Star Section, Norwegian Astronomical Society, PO Box 1029 Blindern, 0315 Oslo, Norway
Kotková, L.;  Astronomical Institute, Academy of Sciences, 251 65 Ondrejov, Czech Republic
Santacana, G.;  Association AstroQueyras, Le Bois de Bardon, Taponnat, 16110 La Rochefoucauld, France
Michelet, J.;  Club d'Astronomie Lyon Ampère, 37 rue Paul Cazeneuve, 69008 Lyon, France
Fauvaud, M.;  Association AstroQueyras, Le Bois de Bardon, Taponnat, 16110 La Rochefoucauld, France
Vugnon, J*-M;  Club Eclipse, 22 rue du Borrégo, Appt 5A4, 75020 Paris, France
Sadsaoud, H.;  CRAAG, Algiers Observatory, BP 63 Bouzareah 16340, Algiers, Algeria
Aliouane, S.;  CRAAG, Algiers Observatory, BP 63 Bouzareah 16340, Algiers, Algeria
Grigahcéne, Z. C.;  CRAAG, Algiers Observatory, BP 63 Bouzareah 16340, Algiers, Algeria
Martín-Ruíz, S.;  Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain
Amado, P. J.;  Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain
Suárez, J. C.;  Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain
Moya, A.;  Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain
Kucáková, H.;  Observatory and Planetarium of Johann Palisa, VSB-Technical University, Listopadu 15, 708 33 Ostrava-Poruba, Czech Republic
Kocián, R.;  Observatory and Planetarium of Johann Palisa, VSB-Technical University, Listopadu 15, 708 33 Ostrava-Poruba, Czech Republic
Truparová, K.;  Observatory and Planetarium of Johann Palisa, VSB-Technical University, Listopadu 15, 708 33 Ostrava-Poruba, Czech Republic
Avdibegovic, A.;  Astronomical Institute, Charles University Prague, V Holesovickach 2, 180 00 Praha 8, Czech Republic
Blazek, M.;  Astronomical Institute, Charles University Prague, V Holesovickach 2, 180 00 Praha 8, Czech Republic
Kliner, J.;  Astronomical Institute, Charles University Prague, V Holesovickach 2, 180 00 Praha 8, Czech Republic
Zasche, P.;  Astronomical Institute, Charles University Prague, V Holesovickach 2, 180 00 Praha 8, Czech Republic
Vilásek, M.;  Observatory and Planetarium of Johann Palisa, VSB-Technical University, Listopadu 15, 708 33 Ostrava-Poruba, Czech Republic
Bartosíková, S.;  Observatory and Planetarium of Johann Palisa, VSB-Technical University, Listopadu 15, 708 33 Ostrava-Poruba, Czech Republic
Yasarsoy, B.;  Ege University Observatory, 35100 Bornova, Izmir, Turkey
Ulusoy, C.;  Ege University Observatory, 35100 Bornova, Izmir, Turkey
Graham, K. A.;  American Association of Variable Star Observers, 25 Birch St., Cambridge, MA 02138, USA
Nicholson, M. P.;  American Association of Variable Star Observers, 25 Birch St., Cambridge, MA 02138, USA
Trondal, O.;  Variable Star Section, Norwegian Astronomical Society, PO Box 1029 Blindern, 0315 Oslo, Norway
Yesilyaprak, C.;  Akdeniz University, Art & Science Faculty, Dep. of Physics, Antalya, Turkey
Coker, D.;  Ankara University, Science Faculty, Department of Astronomy and Space Sciences, 06100 Ankara, Turkey
More authors (40 more) Less
Language :
English
Title :
The field high-amplitude SX Phoenicis variable BL Camelopardalis: results from a multisite photometric campaign. I. Pulsation
Publication date :
01 August 2007
Journal title :
Astronomy and Astrophysics
ISSN :
0004-6361
eISSN :
1432-0746
Publisher :
EDP Sciences, Les Ulis, France
Volume :
471
Pages :
255-264
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
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