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Exocomets in the circumstellar gas disk of HD 172555
The source HD172555 is a young A7V star surrounded by a debris disk with a gaseous component.
Here, we present the detection of variable absorption features detected simultaneously in the Ca II K and H doublet lines (at 3,933 and 3,968 Angstrom). We identified the presence of these absorption signatures at four different epochs in the 129 HARPS high-resolution spectra gathered between 2004 and 2011.
These transient absorption features are most likely due to Falling Evaporating Bodies (FEBs, or exocomets) that produce absorbing gas observed transiting in front of the central star. We also detect a stable Ca II absorption component at the star’s radial velocity. With no corresponding detection in the Na I line, the resulting very low upper limit for the NaI/CaII ratio suggests that this absorption is due to circumstellar gas.
Flavien Kiefer, Alain Lecavelier des Etangs, Jean-Charles Augereau, Alfred Vidal-Madjar, Anne-Marie Lagrange, Herve Beust (Submitted on 7 Jan 2014)
Comments: Accepted for publication in Astronomy&Astrophysics Letters
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:1401.1365 [astro-ph.EP] (or arXiv:1401.1365v1 [astro-ph.EP] for this version)
Submission history From: Flavien Kiefer [view email] [v1] Tue, 7 Jan 2014 13:26:21 GMT (593kb)