{ "id": "1609.06611", "version": "v1", "published": "2016-09-21T15:59:22.000Z", "updated": "2016-09-21T15:59:22.000Z", "title": "A Search for Mass Loss on the Cepheid Instability Strip using HI 21-cm Line Observations", "authors": [ "L. D. Matthews", "M. Marengo", "N. R. Evans" ], "comment": "Accepted to AJ; 16 pages", "categories": [ "astro-ph.SR", "astro-ph.GA" ], "abstract": "We present the results of a search for HI 21-cm line emission from the circumstellar environments of four Galactic Cepheids (RS Pup, X Cyg, $\\zeta$ Gem, and T Mon) based on observations with the Karl G. Jansky Very Large Array. The observations were aimed at detecting gas associated with previous or ongoing mass loss. Near the long-period Cepheid T Mon, we report the detection of a partial shell-like structure whose properties appear consistent with originating from an earlier epoch of Cepheid mass loss. At the distance of T Mon, the nebula would have a mass (HI+He) of $\\sim0.5M_{\\odot}$, or $\\sim$6\\% of the stellar mass. Assuming that one-third of the nebular mass comprises swept-up interstellar gas, we estimate an implied mass-loss rate of ${\\dot M}\\sim (0.6-2)\\times10^{-5} M_{\\odot}$ yr$^{-1}$. No clear signatures of circumstellar emission were found toward $\\zeta$ Gem, RS Pup, or X Cyg, although in each case, line-of-sight confusion compromised portions of the spectral band. For the undetected stars, we derive model-dependent $3\\sigma$ upper limits on the mass-loss rates, averaged over their lifetimes on the instability strip, of $<(0.3-6)\\times10^{-6} M_{\\odot}$ yr$^{-1}$ and estimate the total amount of mass lost to be less than a few per cent of the stellar mass.", "revisions": [ { "version": "v1", "updated": "2016-09-21T15:59:22.000Z" } ], "analyses": { "keywords": [ "mass loss", "cepheid instability strip", "line observations", "mass comprises swept-up interstellar gas", "nebular mass comprises swept-up interstellar" ], "note": { "typesetting": "TeX", "pages": 16, "language": "en", "license": "arXiv", "status": "editable" } } }