Abstract
The identification of transiting planets candidates and their a posteriori confirmation and characterization by means of spectroscopic follow-up is allowing us to study the internal physics of these planets. Here we briefly discuss the spectroscopic follow-up of the OGLE transiting candidates carried out at the ESO/VLT.
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Melo, C. et al. (2008). Transiting Planets: Follow the FLAMES.... In: Santos, N.C., Pasquini, L., Correia, A.C.M., Romaniello, M. (eds) Precision Spectroscopy in Astrophysics. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-75485-5_40
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DOI: https://doi.org/10.1007/978-3-540-75485-5_40
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