“Thermal” SiO radio line emission towards M-type AGB stars: A probeof circumstellar dust formation and dynamics

Publisher: Edp Sciences

E-ISSN: 1432-0746|411|2|123-147

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.411, Iss.2, 2003-11, pp. : 123-147

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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