Studies of the magnetic field and its structure in the star HD37776 by various authors are discussed. Significant conflicts among these results are noted which suggest that the star has not been definitively studied. The main reason for the erroneous results is the complexity of the magnetic field structure. This leads to difficulties in measuring and interpreting the magnetic field.
Article PDF
Similar content being viewed by others
Avoid common mistakes on your manuscript.
References
Yu. V. Glagolevskij and A. F. Nazarenko, Astrophys. Bull. 72 (2017).
I. B. Thompson and J. D. Landstreet, Astrophys. J. 289, L9 (1985).
D. A. Bohlender, PhD Thesis, Univ. Western Ontario, Canada (1988).
D. A. Bohlender and J. D. Landstreet, Science News, Jan. 27, 1990.
D. Bohlender, in: L. A. Bolona, H. F. Henrichs, and J. M. Le Contel, ed., Pulsation, rotation and mass loss in Early-type stars, IAU Symp., No 162 (1994), p. 155.
E. Gerth, Yu. V. Glagolevskij, and G. Scholz, in: Yu. V. Glagolevskij and I. I. Romanyuk, eds., Stellar magnetic fields, Moscow (1997), p. 67.
E. Gerth and Yu. V. Glagolevskij, in Magnetic fields of chemically peculiar and related stars, Moscow (2000), p. 151.
E. Gerth and Yu. V. Glagolevskij, Bull. SAO, 56, 25 (2003).
I. I. Romanyuk, et al., Bull. SAO, 45, 93 (1998).
V. L. Khokhlova, et al., Astron. Lett. 26, 177 (2000).
Yu. V. Glagolevskij and E. Gerth, Bull. SAO, 51, 84 (2001).
O. Kochukhov, et al., Astrophys. J. 726, 24 (2011).
N. Piskunov and O. Kochukhov, Astron. Astrophys. 381, 736 (2002).
O. Kochukhov and N. Piskunov, Astron. Astrophys. 388, 868 (2002).
J. Braithwait and A. Nordlund, Astron. Astrophys. 450, 1077 (2006).
Yu. V. Glagolevskij and A. F. Nazarenko, Astrophys. Bull. 72, 411 (2017).
Yu. V. Glagolevskij, Astrophys. Bull. 73, 201 (2018).
Yu. V. Glagolevskij, Astrophys. Bull. 71, 43 (2016).
Yu. V. Glagolevskij, Astrophys. Bull. 68, 356 (2013).
Yu. V. Glagolevskij, Astrophysics, 59, 321 (2016).
Yu. V. Glagolevskij, Astrophysics, 57, 204 (2014).
Yu. V. Glagolevskij, Astrophys. Bull. 72, 334 (2017).
D. Moss, IAU Symp. 224, 245 (2004).
A. E. Dudorov, in: G. M. Rudnitskii, ed., Itogi nauki i techniki, Ser. Astronomiya, VINITI, Moscow, Vol. 39, p. 77 (1990).
G. Mathys, S. Hubrig, J. D. Landstreet, et al., Astron. Astrophys. Suppl. Ser. 123, 353 (1997).
G. Preston, Publ. Astron. Soc. Pacif. 83, 571 (1971).
Yu. V. Glagolevskij, Astrophys. Bull. 74, 66 (2019).
Yu. V. Glagolevskij, Astrophys. Bull. 72, 457 (2017).
I. I. Romanyuk, et al., IAU Symp., No. 176, Vienna (1995), p. 153.
T. Ch. Mouschovias and E. V. Paleologou, Astrophys. J. 230, 204 (1979).
Yu. V. Glagolevskij, Astrophysics, 61, 413 (2018).
E. F. Borra and J. D. Landstreet, Astrophys. J. 212, 141 (1977).
Author information
Authors and Affiliations
Corresponding author
Additional information
Translated from Astrofizika, Vol. 62, No. 2, pp. 239-258 (May 2019)
Rights and permissions
About this article
Cite this article
Glagolevskij, Y.V., Nazarenko, A.F. Remarks on the Properties of the Magnetic Field of the Star HD37776. Astrophysics 62, 210–225 (2019). https://doi.org/10.1007/s10511-019-09575-6
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s10511-019-09575-6