Spectroscopic properties of stars with debris discs

Details Spectroscopic properties of stars with debris discs Spectroscopic properties of stars with debris discs

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011jphcs.328a2011m&link_type=abstract

Journal of Physics: Conference Series, Volume 328, Issue 1, pp. 012011 (2011).

Physics

Scientific paper

The question of the origin and evolution of planetary systems is of fundamental importance for astrophysics. Dusty debris discs are signatures of planetary systems and, therefore, constitute valuable tools to provide new light in our understanding of how planetary systems form and evolve. We present the first results of a spectroscopic programme of a sample of stars with debris discs. High-resolution echelle spectra are used to determine metallicities and abundances. Properties of stars with debris discs, are compared with those of stars hosting planets, as well as 'normal' stars.

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