::: 網站導覽 English VersionEnglish 列印友善列印 搜尋說明
研究成果藝廊 > 天文物理理論與觀測整合研究計畫

研究成果藝廊

天文物理理論與觀測整合研究計畫

HIGH-RESOLUTION CO OBSERVATION OF THE CARBON STAR CIT 6
圖片來源: Hyosun Kim, Sheng-Yuan Liu, Naomi Hirano et al. (2015)
HIGH-RESOLUTION CO OBSERVATION OF THE CARBON STAR CIT 6
Radial profiles of the 12CO J = 2–1 (left panel) and 13CO J = 2–1 (right panel) emission of the carbon star CIT6 at its systemic velocity observed by the Submillimeter Array (SMA), the Submillimeter Telescope (SMT), and combined. Results from the calculations with our radiative transfer modeling package (SPARX), as overlaid by green curves, reproduced the observed profile very well.
電話: 886-2-3365-2200 傳真: 886-2-2367-7849
一般事務: asiaa_replace2@_asiaa.sinica.edu.tw 媒體連絡: epo_replace2@_asiaa.sinica.edu.tw
台北市10617羅斯福路四段1號 中央研究院/台灣大學天文數學館11樓