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OB-stars as extreme condition test beds

Published online by Cambridge University Press:  12 July 2011

Joachim Puls ,
Jon O. Sundqvist  and
Jorge G. Rivero González
Joachim Puls
Affiliation:
Universitätssternwarte der Ludwig-Maximilians-Universität München, Scheinerstr. 1, D-81679 München, Germany email: uh101aw@usm.uni-muenchen.de (J.P.)
Jon O. Sundqvist
Affiliation:
Universitätssternwarte der Ludwig-Maximilians-Universität München, Scheinerstr. 1, D-81679 München, Germany email: uh101aw@usm.uni-muenchen.de (J.P.)
Jorge G. Rivero González
Affiliation:
Universitätssternwarte der Ludwig-Maximilians-Universität München, Scheinerstr. 1, D-81679 München, Germany email: uh101aw@usm.uni-muenchen.de (J.P.)
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Abstract

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Massive stars are inherently extreme objects, in terms of radiation, mass loss, rotation, and sometimes also magnetic fields. Concentrating on a (personally biased) subset of processes related to pulsations, rapid rotation and its interplay with mass-loss, and the bi-stability mechanism, we will discuss how active (and normal) OB stars can serve as appropriate laboratories to provide further clues.

Keywords

hydrodynamicsinstabilitiesline: formationstars: abundancesstars: early-typestars: evolutionstars: mass lossstars: oscillationsstars: rotationstars: windsoutflows
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S272: Active OB stars: structure, evolution, mass loss, and critical limits , July 2010 , pp. 554 - 565
Copyright
Copyright © International Astronomical Union 2011

References

Aerts, C., Puls, J., Godart, M., & Dupret, M.-A. 2009, A&A 508, 409Google Scholar
Aerts, C., Lefever, K., Baglin, A., Degroote, P. et al. 2010, A&A (Letters), 513, L11Google Scholar
Benaglia, P., Vink, J. S., Martí, J., Maíz Apellániz, J. et al. 2007, A&A 467, 1265Google Scholar
Bouret, J.-C., Lanz, T., & Hillier, D. J. 2005, A&A 438, 301Google Scholar
Castor, J. I., Abbott, D. C., & Klein, R. I. 1975, ApJ, 195, 157CrossRefGoogle Scholar
Cranmer, S. R. & Owocki, S. P. 1995, ApJ, 440, 308CrossRefGoogle Scholar
Crowther, P. A., Lennon, D. J., & Walborn, N. R. 2006, A&A, 446, 279Google Scholar
Curé, M., Rial, D. F., & Cidale, L. 2005, A&A, 437, 929Google Scholar
Domiciano de Souza, A., Kervella, P., Jankov, S., Abe, L. et al. 2003, A&A (Letters), 407, L47Google Scholar
Evans, C. J., Lennon, D. J., Trundle, C., Heap, S. R. et al. 2004, ApJ, 607, 451CrossRefGoogle Scholar
Evans, C., Hunter, I., Smartt, S., Lennon, D. et al. 2008, The Messenger, 131, 25Google Scholar
Feldmeier, A., Kudritzki, R.-P., Palsa, R., Pauldrach, A. W. A. et al. 1997, A&A, 320, 899Google Scholar
Feldmeier, A., Puls, J., & Pauldrach, A. W. A. 1997, A&A, 322, 878Google Scholar
Fullerton, A. W., Gies, D. R., & Bolton, C. T. 1996, ApJS, 103, 475CrossRefGoogle Scholar
Georgiev, L. N., Hillier, D. J., & Zsargó, J. 2006, A&A, 458, 597Google Scholar
Glatzel, W. 1998, A&A (Letters), 339, L5Google Scholar
Howarth, I. D., Siebert, K. W., Hussain, G. A. J., & Prinja, R. K. 1997, MNRAS, 284, 265CrossRefGoogle Scholar
Hunter, I., Brott, I., Langer, N., Lennon, D. J. et al. 2009, A&A, 496, 841Google Scholar
Kaufer, A., Stahl, O., Prinja, R. K., & Witherick, D. 2006, A&A, 447, 325Google Scholar
Kudritzki, R.-P., Lennon, D. J., & Puls, J. 1995, in: Walsh, J.R. & Danziger, I.J. (eds.), Science with the VLT, Proc. ESO Workshop (Berlin: Springer), p. 246CrossRefGoogle Scholar
Kervella, P. & Domiciano de Souza, A. 2006, A&A, 453, 1059Google Scholar
Lamers, H. J. G. & Pauldrach, A. W. A. 1991, A&A (Letters), 244, L5Google Scholar
Lamers, H. J. G. L. M., Snow, T. P., & Lindholm, D. M. 1995, ApJ, 455, 269CrossRefGoogle Scholar
Langer, N., Heger, A., & Fliegner, J. 1997, in: Bedding, T. R., Booth, A. J., & Davis, J. (eds.), Fundamental stellar properties: The interaction between observation and theory, IAU Symposium 189, p. 343CrossRefGoogle Scholar
Lefever, K., Puls, J., & Aerts, C. 2007, A&A, 463, 1093Google Scholar
Maeder, A. 1999, A&A, 347, 185Google Scholar
Maeder, A. & Meynet, G. 2000, A&A, 361, 159Google Scholar
Madura, T. I., Owocki, S. P., & Feldmeier, A. 2007, ApJ, 660, 687CrossRefGoogle Scholar
Markova, N. & Puls, J. 2008, A&A, 478, 823Google Scholar
Massa, D., Fullerton, A. W., Nichols, J. S., Owocki, S. P. et al. 1995, ApJ (Letters) 452, L53Google Scholar
Meilland, A., Stee, P., Vannier, M., Millour, F. et al. 2007, A&A 464, 59Google Scholar
Meynet, G., Maeder, A., Schaller, G., Schaerer, D. et al. 1994, A&AS, 103, 97Google Scholar
Owocki, S. P., Cranmer, S. R., & Gayley, K. G. 1998, in: Hubert, A. M. & Jaschek, C. (eds.), B[e] stars, Astrophysics and Space Science Library 233, p. 205CrossRefGoogle Scholar
Pamyatnykh, A. A. 1999, AcA, 49, 119Google Scholar
Pauldrach, A. W. A. & Puls, J. 1990, A&A, 237, 409Google Scholar
Pelupessy, I., Lamers, H. J. G. L. M., & Vink, J. S. 2000, A&A, 359, 695Google Scholar
Petrenz, P. & Puls, J. 1996, A&A, 312, 195Google Scholar
Petrenz, P. & Puls, J. 2000, A&A, 358, 956Google Scholar
Prinja, R. K., Massa, D., Fullerton, A. W., Howarth, I. D. et al. 1997, A&A, 318, 157Google Scholar
Puls, J., Kudritzki, R.-P., Herrero, A., Pauldrach, A. W. A. et al. 1996, A&A, 305, 171Google Scholar
Puls, J., Springmann, U. & Lennon, M. 2000, A&AS, 141, 23Google Scholar
Puls, J., Urbaneja, M. A., Venero, R., Repolust, T. et al. 2005, A&A, 435, 669Google Scholar
Puls, J., Markova, N., Scuderi, S., Stanghellini, C. et al. 2006, A&A, 454, 625Google Scholar
Puls, J., Vink, J. S., & Najarro, F. 2008, A&AR, 16, 209Google Scholar
Repolust, T., Puls, J., & Herrero, A. 2004, A&A, 415, 349Google Scholar
Rivero-González, J. 2010, Diploma-Thesis (LMU München)Google Scholar
Saio, H., Kuschnig, R., Gautschy, A., Cameron, C. et al. 2006, ApJ, 650, 1111CrossRefGoogle Scholar
Simón-Díaz, S., Herrero, A., Uytterhoeven, K., Castro, N. et al. 2010, ApJ (Letters) 720, 174CrossRefGoogle Scholar
Sundqvist, J. O., Puls, J., & Feldmeier, A. 2010, A&A, 510A, 11Google Scholar
Sundqvist, J. O., Puls, J., Owocki, S., et al. 2011, in: Williams, P. & Rauw, G. (eds.), The multi-wavelength view of Hot, Massive Stars, 39th Liège International Astrophysical Colloquium, in pressGoogle Scholar
van Belle, G. T. 2010, in: Rivinius, T. & Curé, M. (eds.), The Interferometric View on Hot Stars, Rev. Mexicana AyA Conference Series 38, p. 119Google Scholar
von Zeipel, H. 1924, MNRAS, 84, 665CrossRefGoogle Scholar
Vink, J. S., de Koter, A., & Lamers, H. J. G. L. M. 2000, A&A, 362, 295Google Scholar
Vink, J. S., de Koter, A., & Lamers, H. J. G. L. M. 2001, A&A, 369, 574Google Scholar
Vink, J. S., Davies, B., Harries, T. J., Oudmaijer, R. D. et al. 2009, A&A, 505, 743Google Scholar
Vink, J. S., Brott, I., Gräfener, G., Langer, N. et al. 2010, A&A (Letters), 512, L7Google Scholar
Waelkens, C., Aerts, C., Kestens, E., Grenon, M. et al. 1998, A&A, 330, 215Google Scholar
Wende, S., Glatzel, W., & Schuh, S. 2008, in: Werner, A. & Rauch, T. (eds.), Hydrogen-Deficient Stars, ASP-CS 391, p. 319Google Scholar
Zahn, J.-P. 1992, A&A, 265, 115Google Scholar
Zickgraf, F.-J., Wolf, B., Leitherer, C., Appenzeller, I. et al. 1986, A&A, 163, 119Google Scholar
Zickgraf, F.-J., Wolf, B., Stahl, O., & Humphreys, R. M. 1989, A&A, 220, 206Google Scholar