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Stars with Discrepant v sin i as Derived from the Ca II 3933 and Mg II 4481 Å Lines. VII. HD9531 (SB), HD31592 (SB2), HD129174 (SB?)

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Abstract

In this paper of the series we analyze three stars listed among stars with discrepant v sin i: HD9531 and HD31592, which also show radial velocity variations inherent to spectroscopic binaries, and HD129174 which is an Mn-type star with a possible magnetic field. In HD9531 we confirm the radial velocity derived fromthe hydrogen lines as well as fromthe Ca II line at 3933 Å as variable. The profile of the calcium line also appears variable, and with the estimated magnetic induction Be = −630 ± 1340 G, this suggests that the abundance of calcium possibly varies over the surface of the star. We identified the lines of the secondary component in the spectrum of HD31592 revealing thus it is an SB2 binary with B9.5V and A0V components. While the primary star rotates with v sin i = 50 km s−1, the secondary star is faster with v sin i = 170 km s−1. We find that only 60% of the Mn lines identified in the spectrum of HD129174 can be fitted with a unique abundance value, whereas the remaining lines are stronger or fainter. We also identified two Xe II lines at 5339.33 Å and 5419.15 Å and estimated their log g f.

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Change history

  • 23 April 2019

    The original paper can be found online at https://doi.org/10.1134/S1990341318030094. The affiliation of the J. Zverko in the original paper was erroneous and need to be corrected. The correct affiliation is:

    <Superscript>1</Superscript>Tatranská Lomnica, 05960 Slovakia

References

  1. D. R. Palmer, E. N. Walker, D. H. P. Jones, and R. E. Wallis, Royal. Obs. Bull. 135, 385 (1968).

    Google Scholar 

  2. S. C. Wolff and G. W. Preston, Astrophys. J. Suppl. 37, 371 (1978).

    Article  ADS  Google Scholar 

  3. J. Zverko, I. Iliev, I. Romanyuk, et al., Astrophysical Bulletin 68, 57 (2013).

    Article  ADS  Google Scholar 

  4. J. Zverko, J. Zˇ ižnŏvský, I. Iliev, et al., Astrophysical Bulletin 66, 325 (2011).

    Article  ADS  Google Scholar 

  5. J. Zverko, I. Iliev, I. Romanyuk, et al., Astrophysical Bulletin 67, 57 (2012).

    Article  ADS  Google Scholar 

  6. J. Zverko, I. Romanyuk, I. Iliev, ey al., Astrophysical Bulletin 68, 442 (2013).

    Article  ADS  Google Scholar 

  7. J. Zverko, I. Romanyuk, I. Iliev, et al., Astrophysical Bulletin 71, 199 (2016).

    Article  ADS  Google Scholar 

  8. J. Zverko, I. Romanyuk, I. Iliev, et al., Astrophysical Bulletin 72, 17 (2017).

    Article  ADS  Google Scholar 

  9. J. Moultaka, S. A. Ilovaisky, P. Prugniel, and C. Soubiran, Publ. Astron. Soc. Pacific 116, 693 (2004).

    Article  ADS  Google Scholar 

  10. V. Panchuk, V. Klochkova, M. Yushkin, and I. Najdenov, Journ. Opt. Technology 76, 87 (2009).

    Article  Google Scholar 

  11. N. E. Piskunov and J. A. Valenti, Astron. and Astrophys. 385, 1095 (2002).

    Article  ADS  Google Scholar 

  12. P. Škoda, ASP Conf. Ser. 101, 187 (1996).

    ADS  Google Scholar 

  13. J. Zverko, J. Žižnŏvský, Z. Mikulášek, and I.Kh. Iliev, Contrib. Astron. Obs. SkalnatéPleso 37, 49 (2007).

    ADS  Google Scholar 

  14. I.Hubeny, T. Lanz, and C. S. Jeffery, Newslett. Analysis Astron. Spectra, No. 20 (1994).

    Google Scholar 

  15. J. Krtička, PhD Thesis, (Masaryk University, Brno,1998) [in Czech language].

    Google Scholar 

  16. F. Castelli and R. L. Kurucz, ASP Conf. Ser. 288, A20 (2003).

    Google Scholar 

  17. N. E. Piskunov, F. Kupka, T. A. Ryabchikova, et al., Astron. and Astrophys. Suppl. 112, 525 (1995).

    ADS  Google Scholar 

  18. T. A. Ryabchikova, N. E. Piskunov, F. Kupka, and W.W. Weiss, Baltic Astronomy 6, 244 (1997).

    ADS  Google Scholar 

  19. F. Kupka, N. E. Piskunov, T. A. Ryabchikova, et al., Astron. and Astrophys. Suppl. 138, 119 (1999).

    Article  ADS  Google Scholar 

  20. F. Kupka, T. A. Ryabchikova, N. E. Piskunov, et al., Baltic Astronomy 9, 590 (2000).

    ADS  Google Scholar 

  21. A. Kramida, Yu. Ralchenko, J. Reader, and NIST ASD Team (2018). NIST Atomic Spectra Database (ver. 5.5.2), [Online. Available: http://pgysics.nist.gov/asd [2018, February 17]. National Institute of Standards and Technology, Gaithersburg,MD.

    Google Scholar 

  22. W. L. Wiese and J. R. Fuhr, J. Phys. Chem. Ref. Data 38, 565 (2009).

    Article  ADS  Google Scholar 

  23. T. Moon and M. M. Dworetsky, Monthly Notices Royal Astron. Soc. 217, 782 (1985).

    Article  Google Scholar 

  24. B. Smalley and M. M. Dworetsky, Astron. and Astrophys. 293, 446 (1995).

    ADS  Google Scholar 

  25. N. Grevesse, M. Asplund, and A. J. Sauval, Space Sci. Rev., 130, 105 (2007).

    Article  ADS  Google Scholar 

  26. R. Komži´k, private communication.

  27. D. Hoffleit and J. H. Warren,Jr., The Bright Star Catalogue, 5th rev. ed. (Astron. Data Center, 1991).

    Google Scholar 

  28. F. Royer, J. Zorec, and A. E. Gomez, Astron. and Astrophys. 463, 671 (2007)

    Article  ADS  Google Scholar 

  29. H. A. Abt, Astrophys. J. 19, 387 (1970).

    Article  ADS  Google Scholar 

  30. S. C. Wolff, Astrophys. J. 222, 556 (1978).

    Article  ADS  Google Scholar 

  31. L. Hric, Astrophys. and Space Sci. 169, 177 (1990).

    Article  ADS  Google Scholar 

  32. G. Hildebrandt, AstronomischeNachrichten 296, 277 (1975).

    ADS  Google Scholar 

  33. I. McDonald, A. A. Zijlstra, and M. L. Boyer, Monthly Notices Royal Astron. Soc. 427, 343 (2012).

    Article  ADS  Google Scholar 

  34. P. North, Astron. and Astrophys. 334, 181 (1998).

    ADS  Google Scholar 

  35. K. Panov and W. Schöneich, Astronomische Nachrichten 297, 177 (1976).

    Article  ADS  Google Scholar 

  36. J. Babel, Astron. and Astrophys. 283, 189 (1994).

    ADS  Google Scholar 

  37. T. Ryabchikova, O. Kochukhov, and S. Bagnulo, Astron. and Astrophys. 480, 811 (2008).

    Article  ADS  Google Scholar 

  38. J. Dommanget and O. Nys, Com. de l’Observ. Royal de Belgique 115, 1 (1994).

    ADS  Google Scholar 

  39. P.C. Schmidtke, J.R. Africano, and R. Quigley, Astron. J. 97, 909 (1989)

    Article  ADS  Google Scholar 

  40. H. A. Abt and N. I. Morrell, Astrophys. J. Suppl. 99, 135 (1995).

    Article  ADS  Google Scholar 

  41. D. L. Crawford, J. V. Barnes, J. C. Golson, and D. P. Hube, Astron. J. 78, 738 (1973).

    Article  ADS  Google Scholar 

  42. J. R.W. Heintze, IAU Symp. 54, 231 (1973).

    ADS  Google Scholar 

  43. A. N. Cox, Allen-s Astrophysical Quantities, 4th ed. (Los Alamos, 1999), p. 381.

    Google Scholar 

  44. H. A. Abt and O. Cardona, Astrophys. J. 276, 266 (1984).

    Article  ADS  Google Scholar 

  45. M. Zboril, Contrib. Astro. Obs. Skalnate Pleso, 16, 47 (1987).

    ADS  Google Scholar 

  46. M. Takada, Publ. Astron. Soc. Japan 31, 473 (1979).

    ADS  Google Scholar 

  47. C.R. Cowley and G. C. L. Aikman, Astrophys. J. 242, 684 (1980).

    Article  ADS  Google Scholar 

  48. S. J. Adelman and D. M. Pyper, Astron. J. 84, 1603 (1979).

    Article  ADS  Google Scholar 

  49. K. M. Strom, Astron. and Astrophys. 2, 182 (1969).

    ADS  Google Scholar 

  50. D. Mihalas and J. L. Henshaw, Astron. J. 144, 25 (1966).

    Article  ADS  Google Scholar 

  51. J. Wm. Montgomery and L. H. Aller, Proc. Nat. Academy Sci. USA 63, 1039 (1969).

    Article  ADS  Google Scholar 

  52. L. Searle, W. T. Lungershausen, and E. L.W. Sargent, Astrophys. J. 145, 141 (1966).

    Article  ADS  Google Scholar 

  53. M. M. Dworetsky, J. L. Persaud, and K. Patel, Monthly Notices Royal Astron. Soc. 385, 1523 (2008).

    Article  ADS  Google Scholar 

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Authors and Affiliations

  1. Istitute of Theoretical Physics and Astrophysics, Tatranská Lomnica, 05960, Slovakia

    J. Zverko

  2. Masaryk University, Brno, 60177, Czech Republic

    J. Zverko

  3. Institute of Astronomy, Bulgarian Academy of Sciences, NAO Rozhen, Sofia, 1784, Bulgaria

    I. Iliev & I. Stateva

  4. Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, 369167, Russia

    I. I. Romanyuk, D. O. Kudryavtsev & E. A. Semenko

Authors
  1. J. Zverko
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  2. I. Iliev
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  3. I. I. Romanyuk
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  4. I. Stateva
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  5. D. O. Kudryavtsev
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  6. E. A. Semenko
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Corresponding author

Correspondence to J. Zverko.

Additional information

Published in Russian in Astrofizicheskii Byulleten’, 2018, Vol. 73, No. 3, pp. 373–385.

The text was submitted by the authors in English.

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Zverko, J., Iliev, I., Romanyuk, I.I. et al. Stars with Discrepant v sin i as Derived from the Ca II 3933 and Mg II 4481 Å Lines. VII. HD9531 (SB), HD31592 (SB2), HD129174 (SB?). Astrophys. Bull. 73, 351–362 (2018). https://doi.org/10.1134/S1990341318030094

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  • DOI: https://doi.org/10.1134/S1990341318030094

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