Magnetic field and chemical composition of the peculiar star HD 10221

Astronomy Letters

Volumn 31, Issue 5, 2005, Pages 327-334

  Glagolevskii, Yu V ^a   Ryabchikova, T A ^b   Chountonov, G A ^a  

^a RUSSIAN ACADEMY OF SCIENCES   (Russian Federation)

^b INSTITUTE OF ASTRONOMY   (Russian Federation)

Author keywords

Star variable and peculiar; Stellar chemical composition

Indexed keywords

EID: 18744388572     PISSN: 10637737     EISSN: None     Source Type: Journal    
DOI: 10.1134/1.1922531     Document Type: Article

References (38)

1. H. A. Abt and N. I. Morrell, Astrophys. J., Suppl. Ser. XXXXXX 99, 135 (1995).
2. R. Aurière, J. Silvester, G. A. Wade, et al., in Proc. of Stellar Magnetic Fields (Spec. Astrphys. Obs., 2005) (in press).
3. H. W. Babcock, Astrophys. J., Suppl. Ser. XXXXXX 3, 141 (1958).
4. L. A. Balona, Mon. Not. R. Astron. Soc. MNRAA4 268, 119 (1994).
5. P. S. Barklem, N. Piskunov, and O'Mara, Astron. Astrophys. AAEJAF 363, 1091 (2000).
6. F. Castelli, R. G. Gratton, and R. L. Kurucz, Astron. Astrophys. AAEJAF 318, 841 (1997).
7. Yu. V. Glagolevskii, V. D. Bychkov, I. Kh. Iliev, et al., Pis'ma Astron. Zh. PAZHDA 8, 26 (1982)
8. [Sov. Astron. Lett. SALEDW 8, 12 (1982)].
9. Yu. V. Glagolevskii, I. I. Romanyuk, N. M. Chunakova, and V. G. Shtol', Astrofiz. Isslad., Izv. Spets. Astrofiz. Obs. XXXXXX 23, 37 (1986).
10. Yu. V. Glagolevskii, Bull. Spec. Astrophys. Obs. XXXXXX 53, 33 (2002).
11. Yu. V. Glagolevskii and G. A. Chuntonov, Astrofiz. XXXXXX 45, 499 (2002)
12. [Astrophys. ATPYAA 45, 408 (2002)].
13. A. E. Gomez, X. Luri, S. Grenier, et al., Astron. Astrophys. AAEJAF 336, 953 (1998).
14. N. Grevesse and A. J. Sauval, Space. Sci. Rev. XXXXXX 85, 161 (1998).
15. B. Hauck and M. Mermilliod, Astron. Astrophys., Suppl. Ser. XXXXXX 129, 431 (1998).
16. G. Hildebrandt, Astron. Nachr. ASNAAN 296, 277 (1975).
17. H. Holweger, AIP Conf. Proc. APCPCS 598, 23 (2001).
18. A. Kaiser, Commun. Asteroseismol. (2005) (in press).
19. D. O. Kudryavtsev, Magnetic Fields of Chemically Peculiar and Related Stars, in Proc. Int. Conf., Ed. by Yu. V. Glagolevskii and I. I. Romanyuk (Russ. Acad. Sci., Moscow, 2000), p. 84.
20. F. Kupka, N. Piskunov, T. A. Ryabchikova, et al., Astron. Astrophys., Suppl. Ser. XXXXXX 138, 119 (1999).
21. R. L. Kurucz, CD-ROM's 18-23 (1993).
22. Z. Lopez-Garcia and S. J. Adelman, Astron. Astrophys., Suppl. Ser. XXXXXX 107, 353 (1994).
23. T. Moon and M. Dworetsky, Mon. Not. R. Astron. Soc. MNRAA4 217, 305 (1985).
24. R. Napiwotzki, D. Schönberner, and V. Wenske, Astron. Astrophys. AAEJAF 268, 653 (1993).
25. N. Piskunov, Stellar Magnetism Ed. by Yu. V. Glagolevskij and I. I. Romanyuk (Nauka, St. Petersburg, 1992), p. 92.
26. A. J. J. Raassen and P. H. M. Uylings, Astron. Astrophys. AAEJAF 340, 300 (1998).
27. I. Ribas, C. Jordi, J. Torra, and A. Gimenez, Astron. Astrophys. AAEJAF 327, 207 (1997).
28. F. Royer, S. Grenier, M.-O. Baylac, et al., Astron. Astrophys. AAEJAF 393, 897 (2002).
29. T. A. Ryabchikova, N. Piskunov, H. C. Stempels, et al., Phys. Scr., T XXXXXX 83, 1962 (1999).
30. T. Ryabchikova, N. Piskunov, O. Kochukhov, et al., Astron. Astrophys. AAEJAF 384, 545 (2002).
31. T. Ryabchikova, G. A. Wade, and F. LeBlanc, IAU Symp. No. 210: Modelling of Stellar Atmospheres, Ed. by N. Piskunov, W. W. Weiss, and D. F. Gray, (Publ. Astron. Soc. Pac., 2003), p. 301.
32. T. Ryabchikova, F. Leone, O. Kochukhov, and S. Bagnulo, Proc. IAU Symp. No. 224: The A-Star Puzzle, Ed. by J. Zverko, W. W. Weiss, J. Žižňovský, and S. J. Adelman (Cambridge Univ. Press, 2004) (in press).
33. T. Ryabchikova, F. Leone, and O. Kochukhov, Astron. Astrophys. (2005) (in press).
34. K. Stȩpień, Astron. Astrophys. AAEJAF 353, 227 (2000).
35. V. Straizis and G. Kuriliene, Astrophys. Space Sci. APSSBE 80, 353 (1981).
36. A. Uesugi and I. Fukuda, Revised Catalogue of Stellar Rotational Velocities (Univ. Kyoto, Kyoto, 1982).
37. G. A. Wade, T. A. Ryabchikova, S. Bagnulo, and N. Piskunov, Astron. Soc. Pac. Conf. Ser. XXXXXX 248, 341 (2001).
38. Z. G. Zhang, S. Svanberg, P. Palmeri, et al., Mon. Not. R. Astron. Soc. MNRAA4 334, 1 (2002).