Zobrazeno 1 - 10
of 87
pro vyhledávání: '"Kyung Won, Suh"'
Autor:
Jang-Ho Lim, Jaeheon Kim, Se-Hyung Cho, Hyosun Kim, Dong-Hwan Yoon, Seong-Min Son, Kyung-Won Suh
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 275, Iss 2, p 20 (2024)
We present the results from long-term simultaneous monitoring observations of SiO and H _2 O masers toward the Mira variable star WX Serpentis. This study has been conducted with 21 m single-dish radio telescopes of the Korean VLBI Network from 2009
Externí odkaz:
https://doaj.org/article/c8f9f878a3a742789ce57b0f67ec8b72
Autor:
Kyung-Won Suh
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 272, Iss 1, p 16 (2024)
We explore the characteristics of carbon stars within our Galaxy through a comprehensive analysis of observational data spanning visual and infrared (IR) bands. Leveraging data sets from IRAS, the Infrared Space Observatory, Akari, the Midcourse Spac
Externí odkaz:
https://doaj.org/article/e9fbf715ec1d4d9d8ce945b151f48f08
Autor:
Kyung-Won Suh
Publikováno v:
Journal of Astronomy and Space Sciences, Vol 33, Iss 2, Pp 119-126 (2016)
To reproduce the spectral energy distributions (SEDs) of young stellar objects (YSOs), we perform radiative transfer model calculations for the circumstellar dust disks with various shapes and many dust species. For eight sample objects of T Tauri
Externí odkaz:
https://doaj.org/article/935b30190c0f42158be5e8571daa7d18
Autor:
Kyung-Won Suh, Young-Joo Kwon
Publikováno v:
Journal of Astronomy and Space Sciences, Vol 28, Iss 4, Pp 253-260 (2011)
To reproduce the multiple broad peaks and the fine spectral features in the spectral energy distributions (SEDs) of T Tauri stars, we model dust around T Tauri stars using a radiative transfer model for multiple isothermal circumstellar dust shells
Externí odkaz:
https://doaj.org/article/8a4dc99b54084078abce196319bed232
Autor:
Young-Joo Kwon, Kyung-Won Suh
Publikováno v:
Journal of Astronomy and Space Sciences, Vol 27, Iss 4, Pp 279-288 (2010)
To study properties of the pulsation in the infrared emission for long period variables, we have collected and analyzed the infrared observational data at M band for 12 OH/IR stars. We present the light curves using the data that cover about 30 yea
Externí odkaz:
https://doaj.org/article/b947ff4caa134f4298e93046940998a4
Autor:
Kyung-Won Suh, Young-Joo Kwon
Publikováno v:
Journal of Astronomy and Space Sciences, Vol 26, Iss 3, Pp 279-286 (2009)
To study properties of the variation of the infrared emission of OH/IR stars, we collect and analyze the infrared observational data in K band for nine OH/IR stars. We use the observational data obtained for about three decades including recent data
Externí odkaz:
https://doaj.org/article/0decc4532015474b94c97ee6d3462ba0
Autor:
Kyung-Won Suh
Publikováno v:
Journal of Astronomy and Space Sciences, Vol 25, Iss 4, Pp 329-334 (2008)
We investigate the spectral energy distributions (SEDs) of Massive Young Stellar Objects (MYSOs) using the various infrared observational data including the Infrared Space Observatory (ISO) data. We model the dust envelopes around the stars using a r
Externí odkaz:
https://doaj.org/article/b8c28e44c44b4e3da1aefe6636b42a5a
Autor:
Kyung-Won Suh
Publikováno v:
Journal of Astronomy and Space Sciences, Vol 24, Iss 3, Pp 197-202 (2007)
We present infrared color-color diagrams of AGB stars from the observations at near and mid infrared bands. We compile the observations for hundreds of OH/IR stars and carbon stars using the data from the Midcourse Space Experiment (MSX), the two mic
Externí odkaz:
https://doaj.org/article/6e38364361a34401b6aa89262c276776
Autor:
Kyung-Won Suh
Publikováno v:
Journal of Astronomy and Space Sciences, Vol 23, Iss 4, Pp 303-310 (2006)
We model the aspherical dust envelopes around O-rich AGB stars. We perform the radiative transfer model calculations for axisymmetric dust distributions. We simulate what could be observed from the aspherical dust envelopes around O-rich AGB stars by
Externí odkaz:
https://doaj.org/article/8699b5968a0b476687e8d2b003e6ecd4
Autor:
Kyung-Won Suh
Publikováno v:
Journal of Astronomy and Space Sciences, Vol 23, Iss 1, Pp 11-18 (2006)
We have modeled dust envelopes around silicate carbon stars using optical properties for a mixture of amorphous carbon and silicate dust grains paying close attention to the infrared observations of the stars. The 4 stars show various properties in c
Externí odkaz:
https://doaj.org/article/18cef9fba7ac420ca7b7a161034f9fb1