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Atmospheric parameters of the B-supergiant HD 198478 from the UV spectra


Jurkić, Tomislav; Sarta Deković, Mariza; Kotnik-Karuza, Dubravka; Dominis-Prester, Dijana
Atmospheric parameters of the B-supergiant HD 198478 from the UV spectra // Astrophysics and space science, 335 (2011), 1; 113-120 doi:10.1007/s10509-011-0637-6 (međunarodna recenzija, članak, znanstveni)


Naslov
Atmospheric parameters of the B-supergiant HD 198478 from the UV spectra

Autori
Jurkić, Tomislav ; Sarta Deković, Mariza ; Kotnik-Karuza, Dubravka ; Dominis-Prester, Dijana

Izvornik
Astrophysics and space science (0004-640X) 335 (2011), 1; 113-120

Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni

Ključne riječi
Line: profiles; stars: fundamental parameters; stars: supergiants; techniques: spectroscopic; ultraviolet: stars

Sažetak
We determined atmospheric parameters of the Galactic early B-supergiant HD198478 (55 Cyg) from the UV silicon lines taken from the high-resolution 1150-1980 angstrems IUE spectra. TLUSTY numerical code was used to model the stellar atmosphere and to determine the temperature and surface gravity assuming a non-LTE plane parallel hydrostatic stellar atmosphere with microturbulence. The synthesized spectra were broadened by the IUE instrumental profile, rotational and macroturbulent velocity with ROTIN numerical code. The silicon 1264, 1309, 1312, 1417 and 1294-1303 angstrems multiplet lines of different stages of ionization (Si II and Si III) were modeled, leading to the temperature, surface gravity, rotational and macroturbulent velocity values. Our results have shown that the line broadening cannot be explained by rotational velocity only, but additional macroturbulent velocity component should be taken into account. HD 198478 shows a significant degeneracy in velocity, which means that the individual contributions of the macroturbulence and rotation in the total velocity broadening cannot be distinguished. Adequate fit of TLUSTY models to the observed non-resonant silicon lines suggests that the non-LTE plane-parallel hydrostatic stellar model without wind contribution can be used to explain such lines. We have obtained similar results using the HST STIS spectra in the same procedure, showing that the IUE spectra, despite their lacking quality compared to the STIS spectra, are reliable enough in determination of the B supergiants' photospheric parameters.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Projekt / tema
316-0000000-2824 - Dijagnostika i fizička svojstva cirkumstelarne tvari (Dubravka Kotnik-Karuza, )

Ustanove
Sveučilište u Rijeci - Odjel za fiziku

Časopis indeksira:


  • Current Contents Connect (CCC)
  • Web of Science Core Collection (WoSCC)
    • Science Citation Index Expanded (SCI-EXP)
    • SCI-EXP, SSCI i/ili A&HCI
  • Scopus


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