Why observe AGB stars at mid-IR wavelengths from Dome C?

Publisher: Edp Sciences

E-ISSN: 1638-1963|33|issue|297-300

ISSN: 1633-4760

Source: EAS Publications Series, Vol.33, Iss.issue, 2008-11, pp. : 297-300

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

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Abstract