Further constraints on the presence of a debris disk in the multiplanet system Gliese 876
Shankland, Paul, Blank, David L., Boboltz, D.A., Lazio, T.J., and White, Graeme L. (2008) Further constraints on the presence of a debris disk in the multiplanet system Gliese 876. Astronomical Journal, 135 (6). pp. 2194-2198.
|PDF (Published version) - Repository staff only - Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader|
View at Publisher Website: http://dx.doi.org/10.1088/0004-6256/135/...
Using both the Very Large Array (VLA) at 7 mm wavelength, and the Australia Telescope Compact Array (ATCA) at 3 mm, we have searched for microwave emission from cool dust in the extrasolar planetary system Gliese 876 (Gl 876). Having detected no emission above our 3σ detection threshold of 135 μJy, we rule out any dust disk with either a mass greater than 0.0006 M ⊕ or less than ~250 AU across. This result improves on previous detection aperture thresholds by an order of magnitude, and it has some implications for the dynamical modeling of the system. It also is consistent with the Greaves et al. hypothesis that relates the presence of a debris disk to close-in planets. Due to the dust-planetesimal relationship, our null result may also provide a constraint on the population or composition of the dust and small bodies around this nearby M dwarf.
|Item Type:||Article (Refereed Research - C1)|
|Keywords:||circumstellar matter; Kuiper Belt; planetary systems; planets and satellites: general; stars: individual (Gl 876)|
|FoR Codes:||02 PHYSICAL SCIENCES > 0201 Astronomical and Space Sciences > 020102 Astronomical and Space Instrumentation @ 100%|
|SEO Codes:||97 EXPANDING KNOWLEDGE > 970102 Expanding Knowledge in the Physical Sciences @ 100%|
|Deposited On:||17 Dec 2009 14:48|
|Last Modified:||18 Oct 2013 00:43|
Last 12 Months: 0
|Citation Counts with External Providers:|
Repository Staff Only: item control page