LkHα 330: Evidence for Dust Clearing through Resolved Submillimeter Imaging
| Autor: | Geoffrey A. Blake, Chunhua Qi, Joanna M. Brown, David J. Wilner, C. P. Dullemond |
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| Rok vydání: | 2008 |
| Předmět: |
Physics
Solid particle Spatially resolved Astronomy Spectral density Astronomy and Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics Planetary system Submillimeter Array Grain growth Space and Planetary Science High spatial resolution Astrophysics::Solar and Stellar Astrophysics Circumstellar dust Astrophysics::Earth and Planetary Astrophysics Astrophysics::Galaxy Astrophysics |
| Zdroj: | The Astrophysical Journal. 675:L109-L112 |
| ISSN: | 1538-4357 0004-637X |
| DOI: | 10.1086/533464 |
| Popis: | Mid-infrared spectrophotometric observations have revealed a small subclass of circumstellar disks with spectral energy distributions (SEDs) suggestive of large inner gaps with low dust content. However, such data provide only an indirect and model-dependent method of finding central holes. We present here the direct characterization of a 40 AU radius inner gap in the disk around LkHα 330 through 340 GHz (880 μm) dust continuum imaging with the Submillimeter Array (SMA). This large gap is fully resolved by the SMA observations and mostly empty of dust with less than 1.3 × 10^−6 M☉ of solid particles inside of 40 AU. Gas (as traced by accretion markers and CO M-band emission) is still present in the inner disk and the outer edge of the gap rises steeply—features in better agreement with the underlying cause being gravitational perturbation than a more gradual process such as grain growth. Importantly, the good agreement of the spatially resolved data and spectrophotometry-based model lends confidence to current interpretations of SEDs with significant dust emission deficits as arising from disks with inner gaps or holes. Further SED-based searches can therefore be expected to yield numerous additional candidates that can be examined at high spatial resolution. |
| Databáze: | OpenAIRE |
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