A method to detect H$_{2}$ in the atmosphere of transiting extrasolar planets using the EUV spectrum

Publisher: Edp Sciences

E-ISSN: 1432-0746|474|1|301-306

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.474, Iss.1, 2007-10, pp. : 301-306

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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