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Abstrakty
We aimed to verify the nature and derive the basic parameters of the symbiotic star candidate [JD2002] 11. For this purpose, we obtained and analyzed an X-Shooter spectrum of [JD2002] 11. We also used optical and infrared photometry available for the object. Emission-line diagnostic ratios are characteristic of a dusty type symbiotic star and reveal a two-component nebula (low- and high-density). The spectral energy distribution is well fitted with a two-component black body spectrum with the respective temperatures of 1150 K and 600 K. The total luminosity of 3000 L⊙ is consistent with the expected luminosity of a typical Mira star, embedded in an optically thick dust shell. We conclude that [JD2002] 11 is the ninth symbiotic star in total and only the second dusty type symbiotic star discovered in the Small Magellanic Cloud.
Czasopismo
Rocznik
Tom
Strony
139--149
Opis fizyczny
Bibliogr. 29 poz., tab., wykr.
Twórcy
autor
- Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716, Warsaw, Poland
autor
- Millennium Institute of Astrophysics, Av. Vicua Mackenna 4860, 782-0436, Macul, Santiago, Chile
- Universidad de Valparaìso, Av. Gran Bretaña 1111, Playa Ancha, Casilla, 5030, Chile
autor
- Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716, Warsaw, Poland
autor
- South African Astronomical Observatory, PO Box 9, Observatory, 7935 Cape Town, South Africa
- outhern African Large Telescope Foundation, PO Box 9, Observatory, 7935 Cape Town, South Africa
autor
- Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
Bibliografia
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Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-1c717254-dfeb-4811-b231-e999c4538c5c