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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 742354.0, MPI für Astronomie / Publikationen_mpia
The results of SED simulations for a young B-Type star IRAS 22150+6109
Authors:Zakhozhay, O. V.; Miroshnichenko, A. S.; Kuratov, K. S.; Zakhozhay, V. A.; Khokhlov, S. A.; Zharikov, S. V.; Manset, N.; Zharikov, S.; Korčáková, D.; Wolf, M.
Place of Publication:San Francisco
Publisher:ASP
Date of Publication (YYYY-MM-DD):2017
Audience:Not Specified
Abstract / Description:We present the results of a spectroscopic analysis and spectral energy distribution (SED) modeling for a young B-type star IRAS 22150+6109. The optical multicolor photometric data were obtained at the Tien-Shan Astronomical Observatory near Almaty, Kazakhstan. Infrared photometry was taken from various sky surveys, such as IRAS, WISE, and AKARI. High-resolution optical spectra were obtained at the 3.6 m Canada-France-Hawaii Telescope (CFHT) and the 2.1 m telescope of the Observatorio Astronómico Nacional San Pedro Martir (OAN SPM). Fundamental parameters of the star are estimated under an assumption that it has a zero-age main-sequence luminosity and a spectral type of B3. The best fit to the SED implies that a large disk is located very far from the star (136 AU) and extended to 850 AU.
External Publication Status:published
Document Type:Other
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/abs/2017ASPC..508..191Z
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