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SCExAO/CHARIS Near-IR High-contrast Imaging and Integral Field Spectroscopy of the HIP 79977 Debris Disk

Goebel, Sean and Currie, Thayne and Guyon, Olivier and Brandt, Timothy D. and Groff, Tyler D. and Jovanovic, Nemanja and Kasdin, N. Jeremy and Lozi, Julien and Hodapp, Klaus and Martinache, Frantz and Grady, Carol and Hayashi, Masa and Kwon, Jungmi and McElwain, Michael W. and Yang, Yi and Tamura, Motohide (2018) SCExAO/CHARIS Near-IR High-contrast Imaging and Integral Field Spectroscopy of the HIP 79977 Debris Disk. Astronomical Journal, 156 (6). Art. No. 279. ISSN 1538-3881. http://resolver.caltech.edu/CaltechAUTHORS:20181128-140625818

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Abstract

We present new, near-infrared (1.1–2.4 μm) high-contrast imaging of the bright debris disk surrounding HIP 79977 with the Subaru Coronagraphic Extreme Adaptive Optics system (SCExAO) coupled with the CHARIS integral field spectrograph. SCExAO/CHARIS resolves the disk down to smaller angular separations of (0farcs11; r ~ 14 au) and at a higher significance than previously achieved at the same wavelengths. The disk exhibits a marginally significant east–west brightness asymmetry in H band that requires confirmation. Geometrical modeling suggests a nearly edge-on disk viewed at a position angle of ~114fdg6 east of north. The disk is best-fit by scattered-light models assuming strongly forward-scattering grains (g ~ 0.5–0.65) confined to a torus with a peak density at r_0 ~ 53–75 au. We find that a shallow outer density power law of α_(out) = −1 to −3 and flare index of β = 1 are preferred. Other disk parameters (e.g., inner density power law and vertical scale height) are more poorly constrained. The disk has a slightly blue intrinsic color and its profile is broadly consistent with predictions from birth ring models applied to other debris disks. While HIP 79977's disk appears to be more strongly forward-scattering than most resolved disks surrounding 5–30 Myr old stars, this difference may be due to observational biases favoring forward-scattering models for inclined disks versus lower inclination, ostensibly neutral-scattering disks like HR 4796A's. Deeper, higher signal-to-noise SCExAO/CHARIS data can better constrain the disk's dust composition.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-3881/aaeb24DOIArticle
https://arxiv.org/abs/1810.09458arXivDiscussion Paper
ORCID:
AuthorORCID
Goebel, Sean0000-0003-3763-2418
Currie, Thayne0000-0002-7405-3119
Guyon, Olivier0000-0002-1097-9908
Brandt, Timothy D.0000-0003-2630-8073
Hodapp, Klaus0000-0003-0786-2140
Martinache, Frantz0000-0003-1180-4138
Kwon, Jungmi0000-0003-2815-7774
Tamura, Motohide0000-0002-6510-0681
Additional Information:© 2018. The American Astronomical Society. Received 2018 May 24; revised 2018 October 15; accepted 2018 October 16; published 2018 November 28. We thank the anonymous referee for helpful suggestions that improved the quality of this work. We also thank Laurent Pueyo for helpful conversations about KLIP forward modeling. T.C. is supported by a NASA Senior Postdoctoral Fellowship. M.T. is partly supported by the JSPS Grant-in-Aid (15H02063). S.G. is supported from NSF award AST 1106391 and NASA Roses APRA award NNX 13AC14G. The development of SCExAO was supported by the JSPS (Grant-in-Aid for Research #23340051, #26220704, #23103002), the Astrobiology Center (ABC) of the National Institutes of Natural Sciences, Japan, the Mt Cuba Foundation and the directors contingency fund at Subaru Telescope. CHARIS was built at Princeton University in collaboration with the National Astronomical Observatory of Japan under a Grant-in-Aid for Scientific Research on Innovative Areas from MEXT of the Japanese government (#23103002). We wish to emphasize the pivotal cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the privilege to conduct scientific observations from this mountain. Facility: Subaru Telescope - (SCExAO, CHARIS). Software: CHARIS Data Reduction Pipeline.
Funders:
Funding AgencyGrant Number
NASA Postdoctoral ProgramUNSPECIFIED
Japan Society for the Promotion of Science (JSPS)15H02063
NSFAST-1106391
NASANNX 13AC14G
Japan Society for the Promotion of Science (JSPS)23340051
Japan Society for the Promotion of Science (JSPS)26220704
Japan Society for the Promotion of Science (JSPS)23103002
National Institutes of Natural Sciences of JapanUNSPECIFIED
Mt. Cuba Astronomical FoundationUNSPECIFIED
Subaru TelescopeUNSPECIFIED
Subject Keywords:circumstellar matter; planetary systems; stars: individual (HIP 79977) ; techniques: high angular resolution
Record Number:CaltechAUTHORS:20181128-140625818
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20181128-140625818
Official Citation:Sean Goebel et al 2018 AJ 156 279
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:91311
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:28 Nov 2018 22:17
Last Modified:28 Nov 2018 22:17

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