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Characterization of the inner disk around HD 141569 A from KECK/NIRC2 L-band vortex coronagraphy
California Institute of Technology/Jet Propulsion Laboratory (NASA), USA.
Jet Propulsion Laboratory (NASA), USA.
Université de Liège, Belgium.
Université de Liège, Belgium.
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2017 (English)In: Astronomical Journal, ISSN 0004-6256, E-ISSN 1538-3881, Vol. 153, no 1, 1-10 p., 44Article in journal (Refereed) Published
Abstract [en]

HD 141569 A is a pre-main sequence B9.5 Ve star surrounded by a prominent and complex circumstellar disk, likely still in a transition stage from protoplanetary to debris disk phase. Here, we present a new image of the third inner disk component of HD 141569 A made in the L′ band (3.8 μm) during the commissioning of the vector vortex coronagraph that has recently been installed in the near-infrared imager and spectrograph NIRC2 behind the W. M. Keck Observatory Keck II adaptive optics system. We used reference point-spread function subtraction, which reveals the innermost disk component from the inner working distance of ;23 au and up to ;70 au. The spatial scale of our detection roughly corresponds to the optical and near-infrared scattered light, thermal Q, N, and 8.6 μm PAH emission reported earlier. We also see an outward progression in dust location from the L′ band to the H  band (Very Large Telescope/ SPHERE image)  to the visible (Hubble Space Telescope (HST)/ STIS image), which is likely indicative of dust blowout. The warm disk component is nested deep inside the two outer belts imaged by HST-NICMOS in 1999 ( at 406 and 245 au, respectively) . We fit our new L′ -band image and spectral energy distribution of HD 141569 A with the radiative transfer code MCFOST. Our best-fit models favor pure olivine grains and are consistent with the composition of the outer belts. While our image shows a putative very faint point-like clump or source embedded in the inner disk, we did not detect any true companion within the gap between the inner disk and the first outer ring, at a sensitivity of a few Jupiter masses.

Place, publisher, year, edition, pages
2017. Vol. 153, no 1, 1-10 p., 44
National Category
Engineering and Technology Astronomy, Astrophysics and Cosmology
URN: urn:nbn:se:uu:diva-311377DOI: 10.3847/1538-3881/153/1/44OAI: oai:DiVA.org:uu-311377DiVA: diva2:1059926
Available from: 2016-12-26 Created: 2016-12-26 Last updated: 2017-01-13

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