Abstract
We observed the bright supergiant ρ Leo (B1 lab) in January–February 2004 using the 6-m telescope of the Special Astrophysical Observatory (Russia) and the 1.8-m telescope of the Bohyunsan Optical Astronomy Observatory (South Korea). 47 spectra with high time resolution (4–10 min), signal-to-noise ratios 300–1000, and spectral resolutions 45 000–60 000 were obtained. We detected variability in the HeI, SiII, SiIII, and NII line profiles, which may be due to rotational modulation of the profiles and photospheric pulsations of ρ Leo. The possible influence of the stellar magnetic field on the line-profile variations is discussed.
Similar content being viewed by others
References
L. Kaper, H. F. Henrichs, A. W. Fullerton, H. Ando, et al., Astron. Astrophys. 327, 281 (1997).
L. Kaper, H. F. Henrichs, J. S. Nichols, J. H. Telting, et al., Astron. Astrophys. 344, 231 (1999).
A. Kaufer, O. Stahl, B. Wolf, et al., Astron. Astrophys. 305, 887 (1996).
S. Lépine, A. F. J. Moffat, Astrophys. J. 514, 909 (1999).
J. A. de Jong, H. F. Henrichs, S. Schrijvers, et al., Astron. Astrophys. 345, 172 (1999).
J. A. de Jong, H. F. Henrichs, L. Kaper, et al., Astron. Astrophys. 368, 601 (2001).
S. M. Kahn, M. A. Leutenegger, J. Cottam, et al., Astron. Astrophys. 365, 365 (2001).
N. A. Miller, J. P. Cassinelli, J. J. MacFarlane, D. H. Cohen, Astroph. J. 499, L195 (2002).
A. F. Kholtygin, D. N. Monin, A. E. Surkov, and S. N. Fabrika, Pis’ma Astron. Zh. 29, 208 (2003) [Astron. Lett. 29, 175 (2003)].
J.-F. Donati, G. A. Wade, J. Babel, et al., Mon. Not. R. Astron. Soc. 326, 1265 (2001).
J.-F. Donati, J. Babel, T. J. Harries, et al., Mon. Not. R. Astron. Soc. 333, 55 (2002).
J.-F. Donati, I. D. Howarth, J.-C. Bouret, et al., Mon. Not. R. Astron. Soc. 365, L6 (2006).
C. Neiner, A. M. Hubert, A. M. Floquet, et al., Astron. Astrophys. 388, 899 (2002).
A. F. Kholtygin, J. Brown, S. Fabrika, and A. Surkov, in Magnetic Stars, Ed. by Yu. V. Glagolevskij, D. O. Kydryavtsev, and I. I. Romanyuk (SAO RAN, 2004), p. 250.
A. F. Kholtygin, G. Galazutdinov, T. E. Burlakov, et al., Astron. Zh. 83, 252 (2006) [Astron. Rep. 50, 220 (2006)].
A. F. Kholtygin, T. E. Burlakova, S. N. Fabrika, et al., Astron. Rep. 50, 887 (2006).
T. Morel, S. V. Marchenko, A. K. Pati, et al., Mon. Not. R. Astron. Soc. 351, 552 (2004).
D. R. Gies and D. L. Lambert, Astrophys. J. 387, 673 (1992).
P. A. Crowther, D. J. Lennon, and N. R. Walborn, Astron. Astrophys. 446, 279 (2006).
A. A. Pamyatnykh, Acta Astron. 49, 189 (1999).
V. E. Panchuk, N. E. Piskunov, V. G. Klochkova, et al., Preprint No. 169, SAO RAN (Special Astrophysical Observatory, Russian Academy of Sciences, Nizhniĭ Arkhyz, 2002).
V. E. Panchuk, V. G. Klochkova, and I. D. Naidenov, Preprint No. 179, SAO RAN (Special Astrophysical Observatory, Russian Academy of Sciences, Nizhniĭ Arkhyz, 2003).
I. D. Howarth, K. W. Siebert, G. A. J. Hussain, and R. K. Prinja, Mon. Not. R. Astron. Soc. 284, 265 (1997).
SIMBAD Astronomical Database (Strasbourg Astronomical Data Center), http://simbad.u-srrasbg.fr/Simbad/.
P. Ballester, Astron. Astrophys. 286, 1011 (1994).
V. S. Shergin, A. Yu. Kniazev, and V. A. Lipovetsky, Astron. Nachr. 317, 95 (1996).
Bohyunsan Echelle Spectrograph (Bohyunsan Optical Astronomy Observatory, Korea), http://www.boao.re.kr/BOES/BOESppt3.files/frame.htm.
G. A. Galazutdinov, Preprint No. 92, SAO RAN (Special Astrophysical Observatory, Russian Academy of Sciences, Nizhniĭ Arkhyz, 1992).
M. Asplund, N. Grevesse, and A. J. Sauval, in Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis, Ed. by F. Bash and T. Barnes (San Francisco: Astron. Soc. Pac.), Astron. Soc. Pac. Conf. Ser. 336, p. astro/ph/0410214.
Th. Rivinius, D. Baade, and S. Stefl, Astron. Astrophys. 411, 229 (2003).
D. H. Roberts, J. Lehar, and J. W. Dreher, Astron. J. 93, 968 (1987).
V. V. Vityazev, Analysis of Irregular Dynamic Series (St. Pterburg. Gos. Univ., St. Petersburg, 2001) [in Russian].
A. F. Kholtygin and A. B. Shneiwais, Astrofizika 48, 87 (2005) [Astrophys. 48, 68 (2005)].
J. H. Telting and C. Schrijvers, Astron. Astrophys., Suppl. Ser. 317, 723 (1997).
V. D. Bychkov, L. V. Bychkova, and J. Madej, Astron. Astrophys. 407, 631B (2003).
S. P. Owocki and S. R. Cranmer, in Radial and Nonradial Pulsations as Probes of Stellar Physics, Ed. by C. Aerts, T. R. Bedding, and J. Christensen-Dalsgaard, Astron. Soc. Pac. Conf. Ser. 259, 512 (1988).
Author information
Authors and Affiliations
Additional information
Original Russian Text © A.F. Kholtygin, S.N. Fabrika, T.E. Burlakova, G.G. Valyavin, G.A. Chuntonov, D.O. Kudryavtsev, D. Kang, M.V. Yushkin, G.A. Galazutdinov, 2007, published in Astronomicheskiĭ Zhurnal, 2007, Vol. 84, No. 11, pp. 1016–1028.
Rights and permissions
About this article
Cite this article
Kholtygin, A.F., Fabrika, S.N., Burlakova, T.E. et al. Microvariability of line profiles in the spectra of OB stars: III. The supergiant ρ LEO. Astron. Rep. 51, 920–931 (2007). https://doi.org/10.1134/S1063772907110054
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1134/S1063772907110054