{ "id": "1107.1786", "version": "v1", "published": "2011-07-09T14:20:44.000Z", "updated": "2011-07-09T14:20:44.000Z", "title": "The Search for Super-saturation in Chromospheric Emission", "authors": [ "Damian J. Christian", "Mihalis Mathioudakis", "Tersi Arias", "Moira Jardine", "David B. Jess" ], "comment": "28 Pages, 6 figures, 1 Table; Accepted in ApJ for Aug 2011", "categories": [ "astro-ph.SR" ], "abstract": "We investigate if the super-saturation phenomenon observed at X-ray wavelengths for the corona, exists in the chromosphere for rapidly rotating late-type stars. Moderate resolution optical spectra of fast rotating EUV- and X-ray- selected late-type stars were obtained. Stars in alpha Per were observed in the northern hemisphere with the Isaac Newton 2.5 m telescope and IDS spectrograph. Selected objects from IC 2391 and IC 2602 were observe in the southern hemisphere with the Blanco 4m telescope and R-C spectrograph at CTIO. Ca II H & K fluxes were measured for all stars in our sample. We find the saturation level for Ca II K at log(L_CaK/L_bol) = -4.08. The Ca II K flux does not show a decrease as a function of increased rotational velocity or smaller Rossby number as observed in the X-ray. This lack of \"super-saturation\" supports the idea of coronal-stripping as the cause of saturation and super-saturation in stellar chromospheres and corona, but the detailed underlying mechanism is still under investigation.", "revisions": [ { "version": "v1", "updated": "2011-07-09T14:20:44.000Z" } ], "analyses": { "keywords": [ "chromospheric emission", "smaller rossby number", "blanco 4m telescope", "moderate resolution optical spectra", "stellar chromospheres" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/738/2/164", "journal": "The Astrophysical Journal", "year": 2011, "month": "Sep", "volume": 738, "number": 2, "pages": 164 }, "note": { "typesetting": "TeX", "pages": 28, "language": "en", "license": "arXiv", "status": "editable", "inspire": 917697, "adsabs": "2011ApJ...738..164C" } } }