Journal
ASTROPHYSICAL JOURNAL
Volume 725, Issue 2, Pages 2392-2400Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/725/2/2392
Keywords
infrared: stars; stars: individual (delta Cephei); stars: mass-loss; stars: variables: Cepheids
Categories
Funding
- NASA [1407]
- Natural Sciences and Engineering Research Council of Canada
- Chandra X-ray Center, NASA [NAS8-03060]
- NSF REU
- Department of Defence ASSURE [0754568]
- Division Of Astronomical Sciences
- Direct For Mathematical & Physical Scien [0754568] Funding Source: National Science Foundation
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We present the discovery of an infrared nebula around the Cepheid prototype delta Cephei and its hot companion HD 213307. Large-scale (similar to 2.1 x 10(4) AU) nebulosity is detected at 5.8, 8.0, 24, and 70 mu m. Surrounding the two stars, the 5.8 and 8.0 mu m emission is largely attributable to polycyclic aromatic hydrocarbon emission swept from the interstellar medium by a wind originating from delta Cephei and/or its companion. Stochastically heated small dust grains are the most likely source of the 24 and 70 mu m extended emission. The 70 mu m emission, in particular, resembles a bow shock aligned in the direction of the proper motion of delta Cephei. This discovery supports the hypothesis that delta Cephei may be currently losing mass, at a rate in the range of approximate to 5 x 10(-9) to 6 x 10(-8) M-circle dot yr(-1).
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