Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-28T03:56:37.840Z Has data issue: false hasContentIssue false
  • English
  • Français

Spectroscopy of be stars

Published online by Cambridge University Press:  11 April 2011

J.-P. Rozelot ,
C. Neiner  and
C. Neiner
C. Neiner*
Affiliation:
LESIA, UMR 8109 du CNRS, Observatoire de Paris-Meudon, 5 place Jules Janssen, 92195 Meudon Cedex, France
Get access

Abstract

This chapter describes non supergiant B-type stars that show emission lines, called Be stars. The emission is caused by the presence of a circumstellar decretion disk. Many physical phenomena are thought to be involved in these stars, such as rapid rotation, pulsations and magnetic fields, and give rise to variations. Spectroscopy is used as a diagnostic tool to study Be stars, by professional astronomers as well as by amateurs.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 47: Astronomical Spectrography for Amateurs , 2011 , pp. 139 - 163
Copyright
© EAS, EDP Sciences, 2011

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Andrillat, A., Jaschek, M., & Jaschek, C., 1990, A&AS, 84, 11
Andrillat, Y., & Fehrenbach, C., 1982, A&AS, 48, 93
Baade, D., 2000, otherinfoin IAU Coll. 175, The Be Phenomenon in Early-Type Stars, ed. Smith, M.A., Henrichs, H.F. & Fabregat, J., ASP Conf. Ser., 214, 178Google Scholar
Balona, L.A., 2000, in IAU Coll. 175, The Be Phenomenon in Early-Type Stars, ed. Smith, M.A., Henrichs, H.F. & Fabregat, J., ASP Conf. Ser., 214, 1Google Scholar
Balona, L.A., Aerts, C., Božić, H. et al., 2001, MNRAS, 327, 1288, B01CrossRef
Banerjee, D.P.K., Rawat, S.D., & Janardhan, P., 2000, A&AS, 147, 229
Bopp, B.W., & Dempsey, R.C., 1989, Inf. Bull. Variable Stars, 3387, 1
Briot, D., 1977, A&A, 54, 599
Buil, C., 2001, Atlas of Be stars on the web [http://www.astrosurf.com/buil/us/bestar.htm]
Chandrasekhar, S., 1950, Radiative transfer (Oxford, Clarendon Press, 1950)Google Scholar
Chauville, J., Zorec, J., Ballereau, D., et al., 2001, A&A, 378, 861
Cohen, D.H., Cassinelli, J.P., & Macfarlane, J.J., 1997, ApJ, 487, 867CrossRef
Collins, G.W., 1987, in IAU Colloq. 92, Physics of Be Stars, 3
Dachs, J., Eichendorf, W., Schleicher, H., et al., 1981, A&AS, 43, 27
Divan, L., 1979, in IAU Colloq. 47, Spectral Classification of the Future, 247
Doazan, V., Sedmak, G., Barylak, M., & Rusconi, L., 1991, ESA-SP 1147
Domiciano de Souza, A., Kervella, P., Jankov, S., et al., 2003, A&A, 407, L47
Donati, J.-F., Semel, M., Carter, B.D., Rees, D.E., &Collier Cameron, A., 1997, MNRAS, 291, 658CrossRef
Floquet, M., Hubert, A.M., Hirata, R., et al., 2000, A&A, 362, 1020
Floquet, M., Neiner, C., Janot-Pacheco, E., et al., 2002, A&A, 394, 137
Frémat, Y., Zorec, J., Hubert, A., & Floquet, M., 2005, A&A, 440, 305
Grady, C.A., Bjorkman, K.S., Snow, T.P., et al., 1989, ApJ, 339, 403CrossRef
Gutiérrez-Soto, J., Floquet, M., Samadi, R., et al., 2009, A&A, 506, 133
Hanuschik, R.W., Hummel, W., Sutorius, E., Dietle, O., & Thimm, G., 1996, A&AS, 116, 309
Henrichs, H.F., de Jong, J.A., Donati, J.-F., et al., 2000, in IAU Coll. 175, The Be Phenomenon in Early-Type Stars, ed. Smith, M.A., Henrichs, H.F. & Fabregat, J., ASP Conf. Ser., 214, 324Google Scholar
Hirata, R., & Hubert-Delplace, A.M., 1981, in Pulsating B-Stars, 217
Huat, A., Hubert, A., Baudin, F., et al., 2009, A&A, 506, 95
Hubert, A.M., & Floquet, M., 1998, A&A, 335, 565
Koubský, P., Harmanec, P., Hubert, A.M., et al., 2000, A&A, 356, 913
Mathys, G., 1989, Fund. Cosmic Phys., 13, 143
Neiner, C., Hubert, A.-M., Floquet, M., et al., 2002, A&A, 388, 899
Neiner, C., Hubert, A.-M., Frémat, Y., et al., 2003, A&A, 409, 275
Oudmaijer, R.D. & Drew, J.E., 1999, MNRAS, 305, 166CrossRef
Poeckert, R., Bastien, P., & Landstreet, J.D., 1979, AJ, 84, 812CrossRef
Quirrenbach, A., Bjorkman, K.S., Bjorkman, J.E., et al., 1997, ApJ, 479, 477CrossRef
Rivinius, T., Baade, D., Stefl, S., et al., 1998, A&A, 336, 177
Schrijvers, C., 1999, Ph.D. Thesis, Universiteit van Amsterdam
Secchi, A., 1867, Astron. Nachr., 68, 63CrossRef
Slettebak, A., 1979, Space Science Rev., 23, 541CrossRef
Sonneborn, G., Grady, C.A., Wu, C., et al., 1988, ApJ, 325, 784CrossRef
Srinivasan, K., 1996, Ph.D. Thesis, Bharathidasan University
Stee, P., 2000, in IAU Coll. 175, The Be Phenomenon in Early-Type Stars, ed. Smith, M.A., Henrichs, H.F. & Fabregat, J., ASP Conf. Ser., 214, 129
Steele, I.A., Negueruela, I., & Clark, J.S., 1999, A&AS, 137, 147
Stibbs, D.W.N., 1950, MNRAS, 110, 395CrossRef
Stokes, G.G., 1852, Trans. Cambridge Phil. Soc., 9, 399
Struve, O., 1931, ApJ, 73, 94CrossRef
Telting, J., 1997, Ph.D. Thesis, Universiteit van Amsterdam
Townsend, R.H.D., Owocki, S.P., & Howarth, I.D., 2004, MNRAS, 350, 189CrossRef
Unno, W., Osaki, Y., Ando, H., Saio, H., & Shibahashi, H., 1989, Nonradial oscillations of stars, 2nd ed. (University of Tokyo Press)Google Scholar
Vakili, F., Mourard, D., Stee, P., et al., 1998, A&A, 335, 261
Vogt, S.S., & Penrod, G.D., 1983, ApJ, 275, 661CrossRef
Waters, L.B.F., Marlborough, J.M., van der Veen, W.E.C., Taylor, A.R., & Dougherty, S.M., 1991, A&A, 244, 120