Abstract
We present an optical spectrum of the star V1648 Aql (IRAS19386+0155) obtained at the 6-m SAO RAS telescope with a spectral resolution of R ≥ 60 000. Heliocentric radial velocity was measured from numerous metal absorptions is Vr = 10.18 ± 0.05 km s-1 (VLSR = 18.1 km s-1). We determined the atmospheric, circumstellar, and interstellar components in the profile of the Na I D lines at Vr = 9.2, -3.4, and -12.8 km s-1 respectively. The averaged over 20 identified DIBs velocity Vr = -12.5 ± 0.2 km s-1 coincides with the interstellar Na I component. Weak emissions with an intensity of about 10% of the local continuum level were detected in the spectrum; they are identified as low-excitation metal lines. Their central position, Vr = 8.44 ± 0.28 km s-1, points to the presence of a weak velocity gradient in the upper layers of the stellar atmosphere. Based on the spectroscopic data and taking into account the interstellar and circumstellar reddening, we estimated the star’s luminosity MV ≈ -5m and also obtained the lower estimate of distance d ≥ 1.8 kpc. Using the model atmosphere method, we determined the fundamental parameters and chemical abundances in the atmosphere confirming the status of a post-AGB star for V1648 Aql.
Similar content being viewed by others
References
W. E. C. J. Veen, H. J. Habing, and T. R. Geballe, Astron. and Astrophys. 226, 108 (1989).
B. M. Lews, J. Eder, and Y. Terzian, Astrophys. J. 362, 634 (1990).
B. M. Lewis, Astrophys. J. 533, 959 (2000).
T. M. Gledhill, Monthly Notices Royal Astron. Soc. 356, 883 (2005).
T. Blöcker, Astron. and Astrophys. 297, 727 (1995).
F. Herwig, Annual Rev. Astron. Astrophys. 43, 435 (2005).
M. Di Criscienzo, P. Ventura, D.A Garcìa-Hernàndez, et al., Monthly Notices Royal Astron. Soc. 462, 395 (2016).
N. Liu, R. Gallino, S. Bisterzo, et al., Astrophys. J. 865, 112 (2018).
O. Suarez, P. García-Lario, A. Manchado, et al., Astron. and Astrophys. 458, 173 (2006).
V. P. Arkhipova, N. P. Ikonnikova, and G. V. Komissarova, Astronomy Letters 36, 269 (2010).
B. J. Hrivnak, W. Lu, and K. A. Nault, Astron. J. 149, 184 (2015).
H. J. Brivnak, S. Kwok, and K. M. Volk, Astrophys. J. 331, 832 (1988).
C. B. Pereira, S. Lorenz-Martins, and M. Machado, Astron. and Astrophys. 422, 637 (2004).
V. E. Panchuk, V. G. Klochkova, and M. V. Yushkin, Astronomy Reports 61, 820 (2017).
M. V. Yushkin and V. G. Klochkova, Preprint No. 206, SAO RAS (Special Astrophysical Observatory RAS, 2004).
G. A. Galazutdinov, PreprintNo. 92, SAORAS (Special Astrophysical Observatory RAS, 1992).
V. G. Klochkova, E. L. Chentsov, N. S. Tavolganskaya, and M. V. Shapovalov, Astrophysical Bulletin 62, 162 (2007).
R. E. Molina, S. Giridhar, C. B. Pereira, et al., Revista Mexicana Astronom. Astrofís. 50, 293 (2014).
V. G. Klochkova, Monthly Notices Royal Astron. Soc. 272, 710, (1995).
V. G. Klochkova and V. E. Panchuk, Astronomy Reports 56, 104 (2012).
V. G. Klochkova, V. E. Panchuk, and N. S. Tavolzhanskaya, Astronomy Reports 62, 623 (2018).
P. Jenniskens and F.-X. Désert, Astron. and Astrophys. Suppl. 106, 39 (1994).
R. Luna, N. L. J. Cox, M. A. Satorre, et al., Astron. and Astrophys. 480, 133 (2008).
E. Bakker, E. F. van Dishoeck, L. B. F. M. Waters, and T. Schoenmaker, Astron. and Astrophys. 323, 469 (1997).
V. G. Klochkova, Astrophysical Bulletin 69, 279 (2014).
J. Kos and T. Zwitter, Astrophys. J. 774, 72 (2013).
R. E. Molina, Revista Mexicana Astronom. Astrofís., 54, 397 (2018).
V. G. Klochkova, M. V. Yushkin, E. L. Chentsov, and V. E. Panchuk, Astronomy Reports 46, 139 (2002).
V. G. Klochkova, E. L. Chentsov, and V. E. Panchuk, Astrophysical Bulletin 74, 41 (2019).
Y. Takeda, G. Jeong, and I. Han, Publ. Astron. Soc. Japan id.8 (2018).
T. Blöcker, Astron. and Astrophys. 299, 755 (1995).
V. V. Kovtyukh, N. I. Gorlova, and S. I. Belik, Monthly Notices Royal Astron. Soc. 423, 3268 (2012).
S. B. Vickers, D. J. Frew, O. A. Parker, and I. S. Bojicic, Monthly Notices Royal Astron. Soc. 447, 1673 (2015).
N. E. Piskunov, F. Kupka, T. A. Ryabchikova, et al., Astron. and Astrophys. Suppl. 112, 525 (1995).
F. Kupka, N. E. Piskunov, T. A. Ryabchikova, et al., Astron. and Astrophys. Suppl. 138, 119 (1999).
V. V. Tsymbal, ASP Conf. Ser. 108, 198 (1996).
K. Lodders, in: Principles and Perspectives in Cosmochemistry (Springer-Verlag, Berlin, Heidelberg, 2010), p. 379 (Astrophysics and Space Science Proc.).
T. Sahin, D. Lambert, V. G. Klochkova, and N.S. Tavolganskaya, Monthly Notices Royal Astron. Soc. 410, 612, (2011).
D.A. Garcìa-Hernandez, O. Zamora, A. Yagüe, et al., Astron. and Astrophys. 555, id.L3 (2013).
P. Ventura and F. D’Antona, Astron. and Astrophys. 439, 1075 (2005).
K. Venn, Astrophys. J. 414, 316 (1993).
K. Lind, M. Asplund, P. S. Barklem, and A. K. Belyaev, Astron. and Astrophys. 528, A103 (2011).
J. C. Wheeler, C. Sneden, and J. W. Jr. Truran, Annual Rev. Astron. Astrophys. 27, 279 (1989).
S. Sumangala Rao, S. Giridhar, and D. L. Lambert, Monthly Notices Royal Astron. Soc. 419, 1254, (2012).
C. Sneden, R. G. Cratton, and D. A. Crocker, Astron. and Astrophys. 246, 354 (1991).
T. V. Mishenina, V. V. Kovtyukh, C. Soubiran, et al., Astron. and Astrophys. 396, 189 (2002).
Y. Takeda, H. Taguchi, K. Yoshioka, et al., Publ. Astron. Soc. Japan 59, 1127 (2007).
R. E. Molina, C. B. Pereira, and A. Arellano Ferro, astro-ph-SR. 1901.058 (2019).
V. G. Klochkova, Bull. Spec. Astrophys. Obs. 44, 5 (1997).
H. van Winckel and M. Reyniers, Astron. and Astrophys. 354, 135 (2000).
V. G. Klochkova and V. E. Panchuk, Astronomy Reports 60, 344 (2016).
Funding
The authors thank the Russian Foundation for Basic Research for partial financial support (project 18-02-00029 a).
Author information
Authors and Affiliations
Corresponding author
Additional information
Russian Text © The Author(s), 2019, published in Astrofizicheskii Byulleten’, 2019, Vol. 74, No. 3, pp. 279–290.
Conflict of Interest
The authors declare that there is no conflict of interest regarding the publication of this paper.
Rights and permissions
About this article
Cite this article
Klochkova, V.G., Tavolzhanskaya, N.S. Optical Spectrum of Distant OH/IR Star V1648 Aql (IRAS 19386+0155). Astrophys. Bull. 74, 277–287 (2019). https://doi.org/10.1134/S1990341319030040
Received:
Revised:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1990341319030040