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A search for photometric and spectroscopic evolutionary changes in the young planetary nebula Vy 2-2

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Abstract

The results of long-term photometric and spectroscopic observations of the young compact planetary nebula Vy 2-2 (PNG 045.4-02.7) are presented. The UBV photometry in 1990–2016 has revealed a slight brightness trend in the yearly averaged data, most pronounced in the V band. We have measured the relative fluxes of optical emission lines on the spectrograms taken with the 1.25-m telescope at the Southern Station of the SAI MSU in 1999–2016, estimated the absolute flux in the Hβ line to be F(Hβ) = (2.1 ± 0.4) × 10−12 erg cm−2 s−1, and determined the interstellar extinction constant c(Hβ) = 1.8. The electron temperature and density in the nebula have been estimated from diagnostic line ratios: Te = (10−12) × 103 K and Ne ≥ 105 cm−3. To detect any possible evolutionary changes, we have compared the new observations with the archival data obtained over the entire history of spectroscopic observations of Vy 2-2. No significant changes in the relative intensities of the strongest emission lines and the integrated flux in the Hβ line exceeding the observational errors have been found. We have revealed a tendency for the intensity ratio F(λ4363)/F(λ4959) to decrease with time, which may be related to a decrease in the electron density in the nebula. Based on our photometric and spectroscopic data, we have estimated the luminosity of the central star of Vy 2-2, which corresponds to the evolutionary tracks for the most massive post-AGB stars of the O-rich sequence.

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References

  1. A. Acker, J. Köppen, B. Stenholm, andG. Jasniewicz, Astron. Astrophys. Suppl. Ser. 80, 201 (1989).

    ADS  Google Scholar 

  2. F. J. Ahern, Astrophys. J. 223, 901 (1978).

    Article  ADS  Google Scholar 

  3. W. J. Altenhoff, C. Thum, andH. J. Wendker, Astron. Astrophys. 281, 161 (1994).

    ADS  Google Scholar 

  4. V. P. Arkhipova, E. B. Kostyakova, M. A. Burlak, V. F. Esipov, and N. P. Ikonnikova, Astron. Rep. 58, 702 (2014).

    Article  ADS  Google Scholar 

  5. R. A. Benjamin, E. D. Skillman, and D. P. Smits, Astrophys. J. 514, 307 (1999).

    Article  ADS  Google Scholar 

  6. M. S. Bessell, Publ. Astron. Soc. Pacif. 102, 1181 (1990).

    Article  ADS  Google Scholar 

  7. T. Blöcker, Astron. Astrophys. 299, 755 (1995).

    ADS  Google Scholar 

  8. M. A. Burlak and V. F. Esipov, Astron. Lett. 36, 752 (2010).

    Article  ADS  Google Scholar 

  9. M. A. Burlak and A. Yu. Kniazev, Astron. Lett. 39, 703 (2013).

    Article  ADS  Google Scholar 

  10. H. Christianto and E. R. Seaquist, Astron. J. 115, 2466 (1998).

    Article  ADS  Google Scholar 

  11. R. E. S. Clegg, M. G. Hoare, and J. R. Walsh, in Planetary Nebulae, Proceedings of the IAU Symposium No. 131, Ed. by S. Torres-Peimbert (Int. Astron.Union, Dordrecht, 1989), p. 443.

  12. M. Cohen and M. J. Barlow, Astrophys. J. 193, 401 (1974).

    Article  ADS  Google Scholar 

  13. J. J. Condon and D. L. Kaplan, Astron. Astrophys. Suppl. Ser. 117, 361 (1998).

    Article  ADS  Google Scholar 

  14. L. E. Davis, E. R. Seaquist, and C. R. Purton, Astrophys. J. 230, 434 (1979).

    Article  ADS  Google Scholar 

  15. W. A. Feibelman, Publ. Astron. Soc. Pacif. 105, 595 (1993).

    Article  ADS  Google Scholar 

  16. F. Gleizes, A. Acker, and B. Stenholm, Astron. Astrophys. 222, 237 (1989).

    ADS  Google Scholar 

  17. I. N. Glushneva, V. T. Doroshenko, T. S. Fetisova, T. S. Khruzina, E. A. Kolotilov, L.V. Mossakovskaya, S. L. Ovchinnikov, and I. B. Voloshina, VizieROnline Data Catalog III/208 (1998).

    Google Scholar 

  18. M. Hajduk, P. A. M. vanHoof, K. Gesicki, A. A. Zijlstra, S. K. Gó rny, and M. Gładkowski, Astron. Astrophys. 567, A15 (2014).

    Article  Google Scholar 

  19. M. Hajduk, P. A. M. van Hoof, and A. A. Zijlstra, Astron. Astrophys. 573, A65 (2015).

    Article  Google Scholar 

  20. G. Handler, R. H.M éndez, R. Medupe, R. Costero, P. V. Birch, M. Alvarez, et al., Astron. Astrophys. 320, 125 (1997).

    ADS  Google Scholar 

  21. D. G. Hummer and P. J. Storey,Mon. Not. R. Astron. Soc. 224, 801 (1987).

    Article  ADS  Google Scholar 

  22. J. B. Kaler, Astrophys. J. 160, 887 (1970).

    Article  ADS  Google Scholar 

  23. J. B. Kaler, Astrophys. J. 220, 887 (1978).

    Article  ADS  Google Scholar 

  24. J. B. Kaler, Astrophys. J. 239, 78 (1980).

    Article  ADS  Google Scholar 

  25. L. Kohoutek, Bull. Astron. Inst. Czechosl. 17, 318 (1966).

    ADS  Google Scholar 

  26. L. Kohoutek, Astron. Astrophys. 378, 843 (2001).

    Article  ADS  Google Scholar 

  27. L. N. Kondratyeva, Astron. Astrophys. Trans. 24, 291 (2005).

    Article  ADS  Google Scholar 

  28. J. Ko¨ ppen, A. Acker, and B. Stenholm, Astron. Astrophys. 248, 197 (1991).

    ADS  Google Scholar 

  29. E. B. Kostyakova and V. P. Arhipova, Astron. Rep. 53, 1155 (2009).

    Article  ADS  Google Scholar 

  30. V. Luridiana, C. Morisset, and R. A. Shaw, Astron. Astrophys. 573, 42 (2015).

    Article  ADS  Google Scholar 

  31. V. M. Lyutyi, Soobshch. GAISh 172, 30 (1971).

    Google Scholar 

  32. K. A. Marsh, Astrophys. J. 201, 190 (1975).

    Article  ADS  Google Scholar 

  33. G. Mellema, Astron. Astrophys. 416, 623 (2004).

    Article  ADS  Google Scholar 

  34. R. H. Méndez, A. D. Verga, and A. Kriner, Rev. Mex. Astron. Astrofis. 8, 175 (1983).

    ADS  Google Scholar 

  35. M. M. Miller Bertolami, Astron. Astrophys. 588, A25 (2016).

    Article  ADS  Google Scholar 

  36. R. Minkowski, Publ. Astron. Soc. Pacif. 58, 305 (1946).

    Article  ADS  Google Scholar 

  37. L. F. Miranda and J. Solf, Astron. Astrophys. 252, 331 (1991).

    ADS  Google Scholar 

  38. A. J. Pickles, Publ. Astron. Soc. Pacif. 110, 863 (1998).

    Article  ADS  Google Scholar 

  39. J. P. Phillips, Rev. Mex. Astron. Astrophys. 42, 291 (2006).

    ADS  Google Scholar 

  40. G. Pojmanski, Acta Astron. 52, 397 (2002).

    ADS  Google Scholar 

  41. R. L. Porter, G. J. Ferland, P. J. Storey, and M. J. Detisch, Mon. Not. R. Astron. Soc. 425, L28 (2012).

    Article  ADS  Google Scholar 

  42. R. L. Porter, G. J. Ferland, P. J. Storey, and M. J. Detisch, Mon. Not. R. Astron. Soc. 433, L89 (2013).

    Article  ADS  Google Scholar 

  43. C. R. Purton, P. A. Feldman, and K. A. Marsh, Nature 245, 6 (1973).

    ADS  Google Scholar 

  44. C.R. Purton, P. A. Feldman, K. A. Marsh, D. A. Allen, and A. E. Wright, Mon.Not.R.Astron.Soc. 198, 321 (1982).

    Article  ADS  Google Scholar 

  45. N. A. Razmadze, Sov. Astron. 4, 938 (1960).

    ADS  Google Scholar 

  46. R. Sahai, M. R. Morris, and G. G. Villar, Astron. J. 141, 134 (2011).

    Article  ADS  Google Scholar 

  47. D. J. Schlegel, D. P. Finkbeiner, and M. Davis, Astrophys. J. 500, 525 (1998).

    Article  ADS  Google Scholar 

  48. E. R. Seaquist and L. E.Davis, Astrophys. J. 274, 659 (1983).

    Article  ADS  Google Scholar 

  49. M. J. Seaton, Mon. Not. R. Astron. Soc. 187, 73P (1979).

    Article  ADS  Google Scholar 

  50. R. A. Shaw and J. B. Kaler, Astrophys. J. 295, 537 (1985).

    Article  ADS  Google Scholar 

  51. R. A. Shaw and J. B. Kaler, Astrophys. J. Suppl. 69, 495 (1989).

    Article  ADS  Google Scholar 

  52. D. P. Smits, Mon. Not. R. Astron. Soc. 278, 683 (1996).

    Article  ADS  Google Scholar 

  53. S. Tamura, I. Kazès, and K. M. Shibata, Astron. Astrophys. 232, 195 (1990).

    ADS  Google Scholar 

  54. R. Tylenda, A. Acker, B. Stenholm, and J. Köppen, Astron. Astrophys. Suppl. Ser. 95, 337 (1992).

    ADS  Google Scholar 

  55. R. Tylenda, A. Acker, and B. Stenholm, Astron. Astrophys. Suppl. Ser. 102, 595 (1993).

    ADS  Google Scholar 

  56. E. Vassiliadis and P. R. Wood, Astrophys. J. Suppl. Ser. 92, 125 (1994).

    Article  ADS  Google Scholar 

  57. B. A. Vorontsov-Velyaminov, E. B. Kostyakova, O. D. Dokuchaeva, and V. P. Arkhipova, Sov. Astron. 9, 564 (1965).

    ADS  Google Scholar 

  58. A. N. Vyssotsky, W. J. Miller, and M. E. Walther, Publ. Astron. Soc. Pacif. 57, 314 (1945).

    Article  ADS  Google Scholar 

  59. R. Wesson, X.-W. Liu, and M. J. Barlow, Mon. Not. R. Astron. Soc. 362, 424 (2005).

    Article  ADS  Google Scholar 

Download references

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Correspondence to M. A. Burlak.

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Original Russian Text © V.P. Arkhipova, M.A. Burlak, V.F. Esipov, N.P. Ikonnikova, G.V. Komissarova, 2017, published in Pis’ma v Astronomicheskii Zhurnal, 2017, Vol. 43, No. 12, pp. 911–924.

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Arkhipova, V.P., Burlak, M.A., Esipov, V.F. et al. A search for photometric and spectroscopic evolutionary changes in the young planetary nebula Vy 2-2. Astron. Lett. 43, 831–843 (2017). https://doi.org/10.1134/S1063773717110019

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