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Investigation of Weakly Magnetic CP Stars. I

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Abstract

The magnetic fields of a sample of chemically peculiar stars, in which they had not been detected earlier, are reinvestigated on the basis of our own measurements and literature data. Despite the considerably higher measurement accuracy, again no magnetic fields were detected in any of them. An upper limit on the field of HD 10221 of 40 G was obtained. Despite the weakness of the fields, the parameters characterizing an anomaly in chemical composition correspond to those for strong fields. The same parameters in stars with strong fields generally correspond in value, although they are lower than expected in the case of HD 47152.

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REFERENCES

  1. Yu. V. Glagolevskii (Glagolevskij) and G. A. Chuntonov (Chountonov), Bull. Spec. Astrophys. Obs., 45, 105 (1998).

    Google Scholar 

  2. Yu. V. Glagolevskii, Astron. Zh., 71, 858 (1994).

    Google Scholar 

  3. V. V. Leushin, Yu. V. Glagolevskii (Glagolevskij), and P. North, in: Magnetic Fields of Chemically Peculiar and Related Stars, Yu. V. Glagolevskij and I. I. Romanyuk, eds., Moscow (2000), p. 173.

  4. N. Cramer and A. Maeder, Astron. Astrophys., 41, 111 (1980).

    Google Scholar 

  5. Yu. V. Glagolevskii, V. D. Bychkov, I. Kh. Iliev, I. I. Romanyuk, and N. M. Chunakova, Pis'ma Astron. Zh., 8, 26 (1982).

    Google Scholar 

  6. Yu. V. Glagolevskii, I. I. Romanyuk, N. M. Chunakova, and V. G. Shtol', Izv. Spets. Astrofiz. Obs., 23, 37 (1986).

    Google Scholar 

  7. Yu. V. Glagolevskii and G. P. Tonil'skaya, Izv. Spets. Astrofiz. Obs., 25, 13 (1987).

    Google Scholar 

  8. I. M. Kopylov, Izv. Spets. Astrofiz. Obs., 24, 44 (1987).

    Google Scholar 

  9. D. N. Brown, J. D. Landstreet, and I. A. Thompson, in: Upper Main Sequence CP Stars, Univ. Liege (1981), p. 195.

  10. G. A. Chuntonov (Chountonov), Rep. Spets. Astrofiz. Obs., 36 (1997).

  11. D. O. Kudryavtsev, in: Magnetic Fields of Chemically Peculiar and Related Stars, Yu. V. Glagolevskij and I. I. Romanyuk, eds., Moscow (2000), p. 84.

  12. S. L. S. Shorlin, G. A. Wade, J.-F. Donati, J. D. Landstreet, P. Petit, T. A. A. Sigut, and S. Strasser, Astron. Astrophys. (2002) (in press).

  13. Yu. V. Glagolevskii (Glagolevskij), Bull. Spec. Astrophys. Obs., 53, 33 (2002).

    Google Scholar 

  14. I. I. Romanyuk, in: Magnetic Fields of Chemically Peculiar and Related Stars, Yu. V. Glagolevskij and I. I. Romanyuk, eds., Moscow (2000), p. 18.

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Authors and Affiliations

  1. Special Astrophysical Observatory, Russian Academy of Sciences, Russia

    Yu. V. Glagolevskii & G. A. Chuntonov

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  1. Yu. V. Glagolevskii
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  2. G. A. Chuntonov
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Glagolevskii, Y.V., Chuntonov, G.A. Investigation of Weakly Magnetic CP Stars. I. Astrophysics 45, 408–415 (2002). https://doi.org/10.1023/A:1021842710087

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  • DOI: https://doi.org/10.1023/A:1021842710087

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