Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Trondal, O."'
Autor:
Fauvaud, S., Sareyan, J. -P., Ribas, I., Rodríguez, E., Lampens, P., Klingenberg, G., Farrell, J. A., Fumagalli, F., Simonetti, J. H., Wolf, M., Santacana, G., Zhou, A. -Y., Michel, R., Fox-Machado, L., Alvarez, M., Nava-Vega, A., López-González, M. J., Casanova, V. M., Aceituno, F. J., Scheggia, I., Rives, J. -J., Hintz, E. G., Van Cauteren, P., Helvaci, M., Yesilyaprak, C., Graham, K. A., Král, L., Kocián, R., Kučáková, H., Fauvaud, M., Granslo, B. H., Michelet, J., Nicholson, M. P., Vugnon, J. -M., Kotková, L., Truparová, K., Ulusoy, C., Yasarsoy, B., Avdibegovic, A., Blauzek, M., Kliner, J., Zasche, P., Bartošíková, S., Vilášek, M., Trondal, O., Abbeel, F. Van Den, Behrend, R., Wücher, H.
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 rad
Externí odkaz:
http://arxiv.org/abs/1004.2748
Autor:
Fauvaud, S., Sareyan, J. -P., Ribas, I., Rodriguez, E., Lampens, P., Klingenberg, G., Farrell, J. A., Fumagalli, F., Simonetti, J. H., Wolf, M., Santacana, G., Zhou, A. -Y., Michel, R., Fox-Machado, L., Alvarez, M., Nava-Vega, A., Lopez-Gonzalez, M. J., Casanova, V. M., Aceituno, F. J., Scheggia, I., Rives, J. -J., Hintz, E. G., Van Cauteren, P., Helvaci, M., Yesilyaprak, C., Graham, K. A., Kral, L., Kocian, R., Kucakova, H., Fauvaud, M., Granslo, B. H., Michelet, J., Nicholson, M. P., Vugnon, J. -M., Kotkova, L., Truparova, K., Ulusoy, C., Yasarsoy, B., Avdibegovic, A., Blazek, M., Kliner, J., Zasche, P., Bartosikova, S., Vilasek, M., Trondal, O., Van Den Abbeel, F., Behrend, R., Wuecher, H.
WOS: 000280505000008
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
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______9436::a06cea3b29f8d7d8fb630d7fb8a4e800
https://hdl.handle.net/11454/43750
https://hdl.handle.net/11454/43750
Autor:
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.
WOS: 000248394400032
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-amplit
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-amplit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______9436::98733fde34e6487afdcf043e32cfcfec
https://hdl.handle.net/11454/39399
https://hdl.handle.net/11454/39399
Autor:
Nikolov, G., Sunay Ibryamov, Radeva, V., Kostov, A., Napetova, M., Bacci, P., Fagioli, G., Tesi, L., Brunetto, L., Jaeger, M., Prosperi, E., Prosperi, S., Vollmann, W., Lehmann, G., Knoefel, A., Buzzi, L., Almendros, I., Hasubick, W., Donati, S., Trondal, O., Snodgrass, C., Kadota, K., Abe, H., Seki, T., Rodriguez, D., Vinko, J., Sarneczky, K., Tholen, D. J., Sheppard, S., Nakata, F., Kashuba, V., Gorbanev, Y., Podlesnyak, S., Zhukov, V., Kashuba, S., Stogneeva, I., Baransky, A., Jewitt, D. C., Hui, M. -T, Melia, R., Colazo, C., Durig, D. T., Ikari, Y., Castellano, J., Dupouy, P., Vanssay, J. B., Storey, D., Muller, J. J., Denzau, H., Nicolas, J., Klotz, A., Kugel, F., Rinner, C., Sonka, A., Bel, J., Beck, S., Noel, T., Bryssinck, E., Soulier, J. -F, Diepvens, A., Aledo, J., Shurpakov, S., Dangl, G., Mainzer, A. K., Bauer, J. M., Grav, T., Masiero, J. R., Dailey, J. W., Cutri, R. M., Wright, E. L., Nugent, C., Sonnett, S., Stevenson, R., Tercu, O., Dumitriu, A., Mantero, A., Cervini, I., Hills, K., Takahashi, T., Herald, D., Lister, T., Primak, N., Schultz, A., Goggia, T., Willman, M., Evans, A. J., Banks, L., Blythe, M., Brungard, R., Festler, P., Mcvey, T., Paige, J., Robertson, W., Spitz, G., Brown, G., Byun, C., Cornell, M., Goldberg, M., Klein, A., Parham, J., Ruprecht, J., Ushomirsky, G., Viggh, H., Woods, D., Lau, P. S., Paul, N., Elenin, L., Savanevych, V., Bryukhovetskiy, A., Hug, G., Sherrod, P. C., Sherrod, L. P., Bell, C., Peterson, H., Chapman, A., Martin, J. L., Carrillo, J., Tilley, S. M., Limon, F., Gonzalez, J., Hernandez, J. F., Garcia, F., Benavides, R., Birtwhistle, P., Armengol, F., Morales, M., Arnold, L., Hudin, L., Tsai, S. -H, Chen, T., Liu, J., Teerasak, T., Sato, H., Guido, E., Howes, N., Nicolini, M., Novichonok, A., Urbanik, M., Jacques, C., Pimentel, E., Barros, J., Prystavski, T., Oey, J., Camilleri, P., Williams, H., Maury, A., Bosch, J. -G, Santucho, M., Valero, J., Soldan A, F. C., Linan, G., Williams, G. V.
Publikováno v:
NASA Astrophysics Data System
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::74844f57849bce027823795068c7a871
https://ui.adsabs.harvard.edu/#abs/2014MPEC....O...54N
https://ui.adsabs.harvard.edu/#abs/2014MPEC....O...54N
Akademický článek
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