{ "id": "0911.2470", "version": "v1", "published": "2009-11-13T17:46:33.000Z", "updated": "2009-11-13T17:46:33.000Z", "title": "Galactic Cepheids with Spitzer: I. Leavitt Law and Colors", "authors": [ "M. Marengo", "N. R. Evans", "P. Barmby", "G. Bono", "D. L. Welch", "M. Romaniello" ], "comment": "Accepted by The Astrophysical Journal on Nov 11, 2009", "categories": [ "astro-ph.SR" ], "abstract": "Classical Cepheid variable stars have been important indicators of extragalactic distance and Galactic evolution for over a century. The Spitzer Space Telescope has opened the possibility of extending the study of Cepheids into the mid- and far-infrared, where interstellar extinction is reduced. We have obtained photometry from images of a sample of Galactic Cepheids with the IRAC and MIPS instruments on Spitzer. Here we present the first mid-infrared period-luminosity relations for Classical Cepheids in the Galaxy, and the first ever Cepheid period-luminosity relations at 24 and 70 um. We compare these relations with theoretical predictions, and with period-luminosity relations obtained in recent studies of the Large Magellanic Cloud. We find a significant period-color relation for the [3.6]-[8.0] IRAC color. Other mid-infrared colors for both Cepheids and non-variable supergiants are strongly affected by variable molecular spectral features, in particular deep CO absorption bands. We do not find strong evidence for mid-infrared excess caused by warm (~500 K) circumstellar dust. We discuss the possibility that recent detections with near-infrared interferometers of circumstellar shells around delta Cep, l Car, Polaris, Y Oph and RS Pup may be a signature of shocked gas emission in a dust-poor wind associated to pulsation-driven mass loss.", "revisions": [ { "version": "v1", "updated": "2009-11-13T17:46:33.000Z" } ], "analyses": { "keywords": [ "galactic cepheids", "leavitt law", "variable molecular spectral features", "classical cepheid", "pulsation-driven mass loss" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/709/1/120", "journal": "The Astrophysical Journal", "year": 2010, "month": "Jan", "volume": 709, "number": 1, "pages": 120 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 836819, "adsabs": "2010ApJ...709..120M" } } }