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Dust Around T Tauri Stars

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. We calculate the radiative transfer model SEDs f...

Deskribapen osoa

Gorde:
Xehetasun bibliografikoak
Egile Nagusiak: Kyung-Won Suh, Young-Joo Kwon
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: The Korean Space Science Society 2011-12-01
Saila:Journal of Astronomy and Space Sciences
Gaiak:
Sarrera elektronikoa:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2011/v28n4/OJOOBS_2011_v28n4_253.pdf
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