Log in

Results of Photometric and Spectroscopic Observations of the Young Variable Star V730 Cep

  • Published:
Astronomy Letters Aims and scope Submit manuscript

Abstract

We present the results of our photometric (V RI) and spectroscopic observations of the young variable star V730 Cep (MisV1147) classified by Uemura et al. (2004) as a Herbig Be star. Our photometry confirms the conclusion of the above authors that this star has a complex pattern of variability including periodic or quasi-periodic brightness variations with a period of about 14 days and deep Algol-like minima typical for UX Ori stars. Our spectroscopy shows that the classification of V730 Cep as a Herbig Be star is wrong. Actually, this star has a much lower temperature and belongs to the family of T Tauri stars. This allows us to explain the nature of the unusual photometric activity of V730 Cep based on a combination of two well-known models of variable circumstellar extinction applied to young stars: AA Tau- and UX Oritype variability. It follows from our observations that the color tracks on the V −(V −I) color–magnitude diagram for these models slightly differ: the AA Tau-type variability of circumstellar extinction is caused by larger grains than the UX Ori-type variability. Such a difference can be due to an increase in the characteristic sizes of circumstellar dust as the star is approached and has a simple explanation: small dust grains evaporate faster than large ones.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Subscribe and save

Springer+ Basic
EUR 32.99 /Month
  • Get 10 units per month
  • Download Article/Chapter or Ebook
  • 1 Unit = 1 Article or 1 Chapter
  • Cancel anytime
Subscribe now

Buy Now

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  1. S. H. P. Alencar, G. Basri, L. Hartmann, and N. Calvet, Astron. Astrophys. 440, 595 (2005).

    Article  ADS  Google Scholar 

  2. J. Bouvier, A. Chelli, S. Allain, L. Carrasco, R. Costero, I. Cruz-Gonzalez, C. Dougados, M. Fernández, et al., Astron. Astrophys. 349, 619 (1999).

    ADS  Google Scholar 

  3. J. Bouvier, K. N. Grankin, and S. H. P. Alencar, Astron. Astrophys. 409, 169 (2003).

    Article  ADS  Google Scholar 

  4. A. G. A. Brown, A. Vallenari, T. Prusti, J. H. J. de Bruijne, C. Babusiaux, and C. A. L. Bailer-Jones (Gaia Collab.), ar**v:1804.09365 (2018).

    Google Scholar 

  5. M. Fang, R. van Boekel, W. Wang, A. Carmona, A. Sicilia-Aguilar, and Th. Henning, Astron. Astrophys. 504, 461 (2009).

    Article  ADS  Google Scholar 

  6. U. Finkenzeller and R. Mundt, Astron. Astrophys. Suppl. Ser. 55, 109 (1984).

    ADS  Google Scholar 

  7. J. F. Gameiro, D. F.M. Folha, and P. P. Petrov, Astron. Astrophys. 445, 323 (2006).

    Article  ADS  Google Scholar 

  8. V. P. Grinin, N. N. Kiselev, N. Kh. Minikhulov, and G. P. Chernova, Sov. Astron. Lett. 14, 219 (1988).

    ADS  Google Scholar 

  9. B. Gustafsson, B. Edwardsson, K. Eriksson, U. G. Jorgensen, A. Nordlund, and B. Plez, Astron. Astrophys. 486, 951 (2008).

    Article  ADS  Google Scholar 

  10. W. Herbst, D. K. Herbst, E. J. Grossman, and D. Weinstein, Astron. J. 108, 1906 (1994).

    Article  ADS  Google Scholar 

  11. J. King, Astron. J. 105, 1087 (1993).

    Article  ADS  Google Scholar 

  12. I. S. Potravnov, V. P. Grinin, and D. E. Mkrtichian, ASP Conf. 508, 335 (2017).

    ADS  Google Scholar 

  13. B. Reiphurt, A. Pedrosa, and M. T.V. T. Lago, Astron. Astrophys. Suppl. Ser. 120, 129 (1996).

    ADS  Google Scholar 

  14. M. M. Romanova, G. V. Ustyugova, A. V. Koldoba, and R. V. E. Lovelace, Astrophys. J. 610, 920 (2004).

    Article  ADS  Google Scholar 

  15. L. Siess, E. Dufor, and M. Forestini, Astron. Astrophys. 358, 593 (2000).

    ADS  Google Scholar 

  16. M. Uemura, T. Kato, R. Ishoka, S. Yoshida, K.-I. Kadota, N. Ohkura, A. Henden, O. Pejcha, et al., Publ. Astron. Soc. Jpn. 56, S183 (2004).

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to V. P. Grinin.

Additional information

Original Russian Text © V.P. Grinin, K.A. Antonyuk, I.S. Potravnov, D. Mkrtichian, 2018, published in Pis’ma v Astronomicheskii Zhurnal, 2018, Vol. 44, No. 12, pp. 868–873.

Rights and permissions

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Grinin, V.P., Antonyuk, K.A., Potravnov, I.S. et al. Results of Photometric and Spectroscopic Observations of the Young Variable Star V730 Cep. Astron. Lett. 44, 798–802 (2018). https://doi.org/10.1134/S1063773718120022

Download citation

  • Received:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1134/S1063773718120022

Keywords

Navigation