Zobrazeno 1 - 10
of 36
pro vyhledávání: '"van Helshoecht"'
Autor:
Moździerski, D., Pigulski, A., Kołaczkowski, Z., Michalska, G., Kopacki, G., Carrier, F., Walczak, P., Narwid, A., Stęślicki, M., Fu, J. -N., Jiang, X. -J., Zhang, Ch., Jackiewicz, J., Telting, J., Morel, T., Saesen, S., Zahajkiewicz, E., Bruś, P., Śródka, P., Vučković, M., Verhoelst, T., Van Helshoecht, V., Lefever, K., Gielen, C., Decin, L., Vanautgaerden, J., Aerts, C.
Publikováno v:
A&A 632, A95 (2019)
Asteroseismology offers the possibility of probing stellar interiors and testing evolutionary and seismic models. Precise photometry and spectroscopy obtained during multi-site campaigns on young open clusters allows discovering rich samples of pulsa
Externí odkaz:
http://arxiv.org/abs/1910.11873
Autor:
Saesen, S., Pigulski, A., Carrier, F., Michalska, G., Aerts, C., De Ridder, J., Briquet, M., Handler, G., Kolaczkowski, Z., Acke, B., Bauwens, E., Beck, P. G., Blom, Y., Blommaert, J., Broeders, E., Cherix, M., Davignon, G., Debosscher, J., Degroote, P., Decin, L., Dehaes, S., De Meester, W., Deroo, P., Desmet, M., Drummond, R., Eggen, J. R., Fu, J., Gazeas, K., Gelven, G. A., Gielen, C., Huygen, R., Jiang, X., Kalomeni, B., Kim, S. -L., Kim, D. H., Kopacki, G., Kwon, J. -H., Ladjal, D., Lee, C. -U., Lee, Y. -J., Lefever, K., Leitner, A., Lenz, P., Liakos, A., Lorenz, D., Narwid, A., Niarchos, P., Oestensen, R., Poretti, E., Prins, S., Provencal, J., Antolin, E. Puga, Puschnig, J., Raskin, G., Reed, M. D., Reyniers, M., Schmidt, E., Schmitzberger, L., Spano, M., Steininger, B., Steslicki, M., Uytterhoeven, K., Vanautgaerden, J., Vandenbussche, B., Van Helshoecht, V., Vanhollebeke, E., Van Winckel, H., Verhoelst, T., Vuckovic, M., Waelkens, C., Wolf, G. W., Yakut, K., Zhang, C., Zima, W.
Publikováno v:
Astronomische Nachrichten 331, No. 9/10, 1080 - 1083 (2010)
As a result of the variability survey in Chi Persei and NGC6910, the number of Beta Cep stars that are members of these two open clusters is increased to twenty stars, nine in NGC6910 and eleven in Chi Persei. We compare pulsational properties, in pa
Externí odkaz:
http://arxiv.org/abs/1004.2853
Autor:
Saesen, S., Carrier, F., Pigulski, A., Aerts, C., Handler, G., Narwid, A., Fu, J. N., Zhang, C., Jiang, X. J., Vanautgaerden, J., Kopacki, G., Stȩślicki, M., Acke, B., Poretti, E., Uytterhoeven, K., Gielen, C., Østensen, R., De Meester, W., Reed, M. D., Kołaczkowski, Z., Michalska, G., Schmidt, E., Yakut, K., Leitner, A., Kalomeni, B., Cherix, M., Spano, M., Prins, S., Van Helshoecht, V., Zima, W., Huygen, R., Vandenbussche, B., Lenz, P., Ladjal, D., Antolín, E. Puga, Verhoelst, T., De Ridder, J., Niarchos, P., Liakos, A., Lorenz, D., Dehaes, S., Reyniers, M., Davignon, G., Kim, S. -L., Kim, D. H., Lee, Y. -J., Lee, C. -U., Kwon, J. -H., Broeders, E., Van Winckel, H., Vanhollebeke, E., Waelkens, C., Raskin, G., Blom, Y., Eggen, J. R., Degroote, P., Beck, P., Puschnig, J., Schmitzberger, L., Gelven, G. A., Steininger, B., Blommaert, J., Drummond, R., Briquet, M., Debosscher, J.
CONTEXT: Recent progress in the seismic interpretation of field beta Cep stars has resulted in improvements of the physics in the stellar structure and evolution models of massive stars. Further asteroseismic constraints can be obtained from studying
Externí odkaz:
http://arxiv.org/abs/1001.1116
Autor:
S. Saesen, V. Van Helshoecht, M. Stęślicki, Przemysław Walczak, D. Moździerski, Karolien Lefever, Xiao-Jun Jiang, Jian-Ning Fu, G. Kopacki, A. Narwid, Jason Jackiewicz, Fabien Carrier, Clio Gielen, J. Telting, P. Bruś, P. Śródka, M. Vučković, J. Vanautgaerden, Thierry Morel, E. Zahajkiewicz, Tijl Verhoelst, Leen Decin, Conny Aerts, Andrzej Pigulski, Z. Kołaczkowski, G. Michalska, C. Zhang
Publikováno v:
Astronomy & Astrophysics
Astronomy & Astrophysics, 632, 1-22
Astronomy & Astrophysics, 632, pp. 1-22
Astronomy & Astrophysics, 632, 1-22
Astronomy & Astrophysics, 632, pp. 1-22
Asteroseismology offers the possibility of probing stellar interiors and testing evolutionary and seismic models. Precise photometry and spectroscopy obtained during multi-site campaigns on young open clusters allows discovering rich samples of pulsa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fb1ef68607f70078a71324c06cd2ac9d
Publikováno v:
Journal of Human Hypertension. Jan2002, Vol. 16 Issue 1, p47. 6p.
Autor:
Martin Groenewegen, V. Van Helshoecht
Publikováno v:
Astronomy & Astrophysics. 463:559-565
We have investigated how the K -band magnitude of the red clump $[M_K(RC)]$ depends on age and metallicity, using 2MASS infrared data for a sample of 24 open clusters with known distances. We show that a constant value of $M_K(RC)=-1.57 \pm 0.05$ is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bdd4150a482e65b46b197cf450a45c4d
https://doi.org/10.1051/0004-6361:20052721
https://doi.org/10.1051/0004-6361:20052721
Publikováno v:
Journal of Human Hypertension. 16:47-52
Hypertension remains a major cause of cardiovascular morbidity in Belgium. Information on the prevalence of hypertension in the working population is desirable. A worksite study of hypertension prevalence was carried out in Belgium where 3472 individ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3a875ae5aedfc9800de7428b8d0b5ab6
https://doi.org/10.1038/sj.jhh.1001293
https://doi.org/10.1038/sj.jhh.1001293
Autor:
Saesen, S., Carrier, F., Pigulski, A., Aerts, C., Handler, G., Narwid, A., Fu, J. N., Zhang, C., Jiang, X. J., Kopacki, G., Vanautgaerden, J., Steślicki, M., Acke, B., Poretti, E., Uytterhoeven, K., De Meester, W., Reed, M. D., Kołaczkowski, Z., Michalska, G., Schmidt, E., xd6stensen, R., Gielen, C., Yakut, K., Leitner, A., Kalomeni, B., Prins, S., van Helshoecht, V., Zima, W., Huygen, R., Vandenbussche, B., Lenz, P., Ladjal, E., Puga Antolxedn, E., Verhoelst, T., De Ridder, J., Niarchos, P., Liakos, A., Lorenz, Saesen, Carrier, Pigulski, Aerts, Handler, Narwid, J. N., Zhang, Jiang, X. J., Kopacki, Vanautgaerden, Steślicki, Acke, Poretti, Uytterhoeven, De Meester, Reed, M. D., Kołaczkowski, Michalska, Schmidt, xd6stensen, Gielen, Yakut, Leitner, Kalomeni, Prins, van Helshoecht, Zima, Huygen, Vandenbussche, Lenz, Ladjal, Puga Antolxedn, Verhoelst, De Ridder, Niarchos, Liakos
Publikováno v:
"Communications in Asteroseismology, Vol.158, p. 179 Proceedings of "38th Liege International Astrop.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=erc_________::ecd23de65f2cbbc50f4885ab0de29c99
Autor:
S. Saesen, A. Pigulski, F. Carrier, G. Michalska, C. Aerts, J. De Ridder, M. Briquet, G. Handler, Z. Kołaczkowski, B. Acke, E. Bauwens, P.G. Beck, Y. Blom, J. Blommaert, E. Broeders, M. Cherix, G. Davignon, J. Debosscher, P. Degroote, L. Decin, S. Dehaes, W. De Meester, P. Deroo, M. Desmet, R. Drummond, J.R. Eggen, J. Fu, K. Gazeas, G.A. Gelven, C. Gielen, R. Huygen, X. Jiang, B. Kalomeni, S.-L. Kim, D.H. Kim, G. Kopacki, J.-H. Kwon, D. Ladjal, C.-U. Lee, Y.-J. Lee, K. Lefever, A. Leitner, P. Lenz, A. Liakos, D. Lorenz, A. Narwid, P. Niarchos, R. Østensen, E. Poretti, S. Prins, J. Provencal, E. Puga Antolin, J. Puschnig, G. Raskin, M.D. Reed, M. Reyniers, E. Schmidt, L. Schmitzberger, M. Spano, B. Steininger, M. Stęślicki, K. Uytterhoeven, J. Vanautgaerden, B. Vandenbussche, V. Van Helshoecht, E. Vanhollebeke, H. Van Winckel, T. Verhoelst, M. Vučković, C. Waelkens, G.W. Wolf, K. Yakut, C. Zhang, W. Zima
Publikováno v:
BASE-Bielefeld Academic Search Engine
As a result of the variability survey in Chi Persei and NGC6910, the number of Beta Cep stars that are members of these two open clusters is increased to twenty stars, nine in NGC6910 and eleven in Chi Persei. We compare pulsational properties, in pa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::04f024dafa6294cc74d75be00b4a9d81
http://arxiv.org/abs/1004.2853
http://arxiv.org/abs/1004.2853
Autor:
L. Schmitzberger, P. G. Beck, Jonas Debosscher, R. H. Østensen, S. Dehaes, K. Uytterhoeven, E. Schmidt, Maarten Reyniers, J. Puschnig, Michael D. Reed, S. L. Kim, P. G. Niarchos, Fabien Carrier, Belinda Kalomeni, C.-U. Lee, Conny Aerts, E. Poretti, B. Steininger, J. Vanautgaerden, E. Broeders, V. Van Helshoecht, M. Cherix, W. De Meester, Jian-Ning Fu, R. Drummond, G. A. Gelven, Pieter Degroote, S. Prins, C. Waelkens, Patrick Lenz, B. Vandenbussche, Sophie Saesen, Z. Kołaczkowski, Bram Acke, Yongseok Lee, G. Kopacki, J. R. Eggen, D. Ladjal, W. Zima, H. Van Winckel, Andrzej Pigulski, J. De Ridder, J. A. D. L. Blommaert, J.-H. Kwon, Rik Huygen, M. Stȩślicki, Y. Blom, C. Zhang, Gerald Handler, Clio Gielen, G. Michalska, T. Verhoelst, A. Leitner, M. Spano, Alexios Liakos, A. Narwid, D. Lorenz, D. H. Kim, Xiao-Jun Jiang, Maryline Briquet, E. Puga Antolín, Kadri Yakut, G. Davignon, Gert Raskin, E. Vanhollebeke
Publikováno v:
Astronomy and Astrophysic
Van Winckel, Hans/0000-0001-5158-9327; Liakos, Alexios/0000-0002-0490-1469; Yakut, Kadri/0000-0003-2380-9008; Lee, Chung-Uk/0000-0003-0043-3925; Verhoelst, Tijl/0000-0003-0163-9984; Reed, Michael/0000-0002-2936-4807; Poretti, Ennio/0000-0003-1200-047
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a004f584ca784e40a872ef03f6931e33
http://arxiv.org/abs/1001.1116
http://arxiv.org/abs/1001.1116