Debes, JH; Hoard, DW; Farihi, J; Wachter, S; Leisawitz, DT; Cohen, M; (2012) The wired survey. III. An infrared excess around the eclipsing post-common envelope binary SDSS J030308.35+005443.7. Astrophysical Journal , 759 (1) , Article 37. 10.1088/0004-637X/759/1/37.

Preview

Text Farihi_apj_759_1_37.pdf Download (352kB) | Preview

Abstract

We present the discovery with WISE of a significant infrared excess associated with the eclipsing post-common envelope binary SDSS J030308.35+005443.7, the first excess discovered around a non-interacting white dwarf+main-sequence M dwarf binary. The spectral energy distribution of the white dwarf+M dwarf companion shows significant excess longward of 3μm. A T eff of 8940K for the white dwarf is consistent with a cooling age >2Gyr, implying that the excess may be due to a recently formed circumbinary dust disk of material that extends from the tidal truncation radius of the binary at 1.96 R ⊙ out to <0.8 AU, with a total mass of 1020 g. We also construct WISE and follow-up ground-based near-infrared light curves of the system and find variability in the K band that appears to be in phase with ellipsoidal variations observed in the visible. The presence of dust might be due to (1) material being generated by the destruction of small rocky bodies that are being perturbed by an unseen planetary system or (2) dust condensing from the companion's wind. The high inclination of this system and the presence of dust make it an attractive target for M dwarf transit surveys and long-term photometric monitoring.

Download activity - last month

Export as JSONXMLCSV

Download activity - last 12 months

Export as CSVXMLJSON

Downloads by country - last 12 months

Export as JSONXMLCSV

Archive Staff Only

View Item