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Makale Tam Makale Uluslararası 2010

The field high-amplitude SX Phe variable BL Cam: results from a multisite photometric campaign

S. Fauvaud, J. -P. Sareyan, I. Ribas, E. Rodriguez, P. Lampens, G. Klingenberg, J. A. Farrell, F. Fumagalli, J. H. Simonetti, M. Wolf, G. Santacana, A. -Y. Zhou, R. Michel, L. Fox-Machado, M. Alvarez, A. Nava-Vega, M. J. Lopez-Gonzalez, V. M. Casanova, F. J. Aceituno, I. Scheggia, J. -J. Rives, E. G. Hintz, P. Van Cauteren, M. Helvaci, Cahit Yeşilyaprak, K. A. Graham, L. Kral, R. Kocian, H. Kucakova, M. Fauvaud, B. H. Granslo, J. Michelet, M. P. Nicholson, J. -M. Vugnon, L. Kotkova, K. Truparova, C. Ulusoy, B. Yasarsoy, A. Avdibegovic, M. Blazek, J. Kliner, P. Zasche, S. Bartosikova, M. Vilasek, O. Trondal, F. Van Den Abbeel, R. Behrend, H. Wuecher

ASTRONOMY & ASTROPHYSICS Cilt 515 · 01.06.2010
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Özet

Context. Short-period high-amplitude pulsating stars of Population I (delta Sct stars) and II (SX Phe variables) exist in the lower part of the classical (Cepheid) instability strip. Most of them have very simple pulsational behaviours, only one or two radial modes being excited. Nevertheless, BL Cam is a unique object among them, being an extreme metal-deficient field high-amplitude SX Phe variable with a large number of frequencies. Based on a frequency analysis, a pulsational interpretation was previously given.

Anahtar kelimeler

stars: variables: delta Scuti stars: individual: BL Camelopardalis stars: oscillations binaries: general techniques: photometric LONG-TERM VARIABILITY DELTA-SCUTI STARS STELLAR EVOLUTION PHOENICIS STARS DWARF CEPHEIDS PERIOD CHANGES CAMELOPARDALIS STRAGGLERS PLANETS TRIPLE

Atıf için künye

Fauvaud, S., Sareyan, J. -., Ribas, I., Rodriguez, E., Lampens, P., Klingenberg, G., Farrell, J. A., Fumagalli, F., Simonetti, J. H., Wolf, M., Santacana, G., Zhou, A. -., Michel, R., Fox-Machado, L., Alvarez, M., Nava-Vega, A., Lopez-Gonzalez, M. J., Casanova, V. M., Aceituno, F. J., … Wuecher, H. (2010). The field high-amplitude SX Phe variable BL Cam: results from a multisite photometric campaign. ASTRONOMY & ASTROPHYSICS, 515. https://doi.org/10.1051/0004-6361/201014243

BibTeX
@article{fauvaud2010-61787,
  author = {Fauvaud, S. and Sareyan, J. -P. and Ribas, I. and Rodriguez, E. and Lampens, P. and Klingenberg, G. and Farrell, J. A. and Fumagalli, F. and Simonetti, J. H. and Wolf, M. and Santacana, G. and Zhou, A. -Y. and Michel, R. and Fox-Machado, L. and Alvarez, M. and Nava-Vega, A. and Lopez-Gonzalez, M. J. and Casanova, V. M. and Aceituno, F. J. and Scheggia, I. and Rives, J. -J. and Hintz, E. G. and Van Cauteren, P. and Helvaci, M. and Yeşilyaprak, Cahit and Graham, K. A. and Kral, L. and Kocian, R. and Kucakova, H. and Fauvaud, M. and Granslo, B. H. and Michelet, J. and Nicholson, M. P. and Vugnon, J. -M. and Kotkova, L. and Truparova, K. and Ulusoy, C. and Yasarsoy, B. and Avdibegovic, A. and Blazek, M. and Kliner, J. and Zasche, P. and Bartosikova, S. and Vilasek, M. and Trondal, O. and Van Den Abbeel, F. and Behrend, R. and Wuecher, H.},
  title = {The field high-amplitude SX Phe variable BL Cam: results from a multisite photometric campaign},
  journal = {ASTRONOMY & ASTROPHYSICS},
  year = {2010},
  volume = {515},
  issn = {0004-6361},
  doi = {10.1051/0004-6361/201014243},
  url = {https://akademik.atauni.edu.tr/yayinlar/61787-the-field-high-amplitude-sx-phe-variable-bl-cam-results-from-a-multisite}
}