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The field high-amplitude SX Phoenicis variable BL Camelopardalis: results from a multisite photometric campaign
Rodriguez, E.; Fauvaud, S.; Farrell, J. A.; Zhou, A.-Y.; Sareyan, J.-P.; Lopez-Gonzalez, M. J.; Dupret, M.-A.; Grigahcene, A.; de Ridder, J.; Klingenberg, G.; Wolf, M.; Van Cauteren, P.; Lampens, P.; Martinez, D.; Casanova, V. M.; Aceituno, F. J.; Helvaci, M.; Hintz, E. G.; Kral, L.; Fumagalli, F.; Simonetti, J. H.; Granslo, B. H.; Kotkova, L.; Santacana, G.; Michelet, J.; Fauvaud, M.; Vugnon, J-M; Sadsaoud, H.; Aliouane, A.; Grigahcene, Z. C.; Martin-Ruiz, S.; Amado, P. J.; Suarez, J. C.; Moya, A.; Kucakova, H.; Kocian, R.; Truparova, B.; Avdibegtovic, A.; Blazek, M.; Kliner, J.; Zasche, P.; Vilasek, M.; Bartosikova, S.; Yasarsoy, B.; Ulusoy, C.; Graham, K. A.; Nicholson, M. P.; Trondal, O.; Yesilyaprak, C.; Coker, D.
2007-08-01
Source PublicationASTRONOMY & ASTROPHYSICS
Volume471Issue:1Pages:255-264
AbstractContext. 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.
KeywordStars : Variables : Delta Sct Stars : Individual : Bl Camelopardalis Stars : Oscillations Techniques : Photometric
DOI10.1051/0004-6361:20077514
Indexed BySCI
Language英语
WOS IDWOS:000248394400032
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8911
Collection射电天文研究部
Affiliation1.CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain
2.Assoc AstroQueyras, F-16110 La Rochefoucaid, France
3.GEOS, Grp Europeen Observ, F-28300 Bailleau, Eveque, France
4.Sulphur Flats Observ, Jemez Springs, NM 87025 USA
5.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
6.Observ Cote Azur, F-06304 Nice 4, France
7.Observ Paris, LESIA, F-92190 Meudon, France
8.Algiers Observ, CRAGG, Algiers 16340, Algeria
9.Katholieke Univ Leuven, Inst Sterrekund, B-3001 Heverlee, Belgium
10.Norwegian Astron Soc, N-0315 Oslo, Norway
11.Charles Univ Prague, Inst Astron, Prague 18000 8, Czech Republic
12.Beersel Hills Observ, B Beersel, Belgium
13.Koninklijke Sterrenwacht Belgie, B-1180 Brussels, Belgium
14.Ankara Univ, Fac Sci, Dept Astron & Space Sci, TR-06100 Ankara, Turkey
15.Brigham Young Univ, Dept Phys & Astron, Provo, UT 84602 USA
16.Tech Univ Ostrava, Observ & Planetarium Johann Palisa, CZ-70833 Ostrava, Czech Republic
17.Virginia Polytech Inst & State Univ, Martin Observ, Phys Dep, Blacksburg, VA 24061 USA
18.Acad Sci Czech Republic, Astron Inst, Ondrejov 25165, Czech Republic
19.Club Astron Lyon Ampere, F-69008 Lyon, France
20.Club Eclipse, F-75020 Paris, France
21.Ege Univ Observ, TR-35100 Bornova, Turkey
22.Amer Assoc Variable Star Observers, Cambridge, MA 02138 USA
23.Akdeniz Univ, Art & Sci Fac, Dep Phys, Antalya, Turkey
Recommended Citation
GB/T 7714
Rodriguez, E.,Fauvaud, S.,Farrell, J. A.,et al. The field high-amplitude SX Phoenicis variable BL Camelopardalis: results from a multisite photometric campaign[J]. ASTRONOMY & ASTROPHYSICS,2007,471(1):255-264.
APA Rodriguez, E..,Fauvaud, S..,Farrell, J. A..,Zhou, A.-Y..,Sareyan, J.-P..,...&Coker, D..(2007).The field high-amplitude SX Phoenicis variable BL Camelopardalis: results from a multisite photometric campaign.ASTRONOMY & ASTROPHYSICS,471(1),255-264.
MLA Rodriguez, E.,et al."The field high-amplitude SX Phoenicis variable BL Camelopardalis: results from a multisite photometric campaign".ASTRONOMY & ASTROPHYSICS 471.1(2007):255-264.
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