{ "id": "1605.06777", "version": "v1", "published": "2016-05-22T12:11:09.000Z", "updated": "2016-05-22T12:11:09.000Z", "title": "Constraints on the presence of SiO gas in the debris disk of HD 172555", "authors": [ "T. L. Wilson", "R. Nilsson", "C. H. Chen", "C. M. Lisse", "M. Moerchen", "H. -U. Käufl", "A. Banzatti" ], "comment": "three figures", "categories": [ "astro-ph.SR", "astro-ph.EP" ], "abstract": "We have carried out two sets of observations to quantify the properties of SiO gas in the unusual HD 172555 debris disk: (1) a search for the J=8-7 rotational transition from the vibrational ground state, carried out with the APEX sub-millimeter telescope and heterodyne receiver at 863 microns, and (2) a search at 8.3 microns for the P(17) ro-vibrational transition of gas phase SiO, carried out with VLT/VISIR with a resolution, $\\lambda/\\Delta\\lambda$, of 30000. The APEX measurement resulted in a 3.3 $\\sigma$ detection of an interstellar feature, but only an upper limit to emission at the radial velocity and linewidth expected from HD 172555. The VLT/VISIR result was also an upper limit. These were used to provide limits for the abundance of gas phase SiO, for a range of temperatures. The upper limit from our APEX detection, assuming an 8000\\,K primary star photospheric excitation, falls more than an order of magnitude below the self-shielding stability threshold derived by Johnson et al. (2012). Our results thus favor a solid-state origin for the 8.3 micron feature seen in the Spitzer IRS spectrum of the circumstellar excess emission, and the production of circumstellar O$^+$ and Si$^+$ by SiO UV photolysis. The implications of these estimates are explored in the framework of models of the HD\\,172555 circumstellar disk.", "revisions": [ { "version": "v1", "updated": "2016-05-22T12:11:09.000Z" } ], "analyses": { "keywords": [ "debris disk", "sio gas", "gas phase sio", "upper limit", "constraints" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }