CONSTRAINING the MOVEMENT of the SPIRAL FEATURES and the LOCATIONS of PLANETARY BODIES WITHIN the AB AUR SYSTEM

Jamie R. Lomax; John P. Wisniewski; Carol A. Grady; Michael W. McElwain; Jun Hashimoto; Tomoyuki Kudo; Nobuhiko Kusakabe; Yoshiko K. Okamoto; Misato Fukagawa; Lyu Abe; Wolfgang Brandner; Timothy D. Brandt; Joseph C. Carson; Thayne M. Currie; Sebastian Egner; Markus Feldt; Miwa Goto; Olivier Guyon; Yutaka Hayano; Masahiko Hayashi; Saeko S. Hayashi; Thomas Henning; Klaus W. Hodapp; Akio Inoue; Miki Ishii; Masanori Iye; Markus Janson; Ryo Kandori; Gillian R. Knapp; Masayuki Kuzuhara; Jungmi Kwon; Taro Matsuo; Satoshi Mayama; Shoken Miyama; Munetake Momose; Jun Ichi Morino; Amaya Moro-Martin; Tetsuo Nishimura; Tae Soo Pyo; Glenn H. Schneider; Eugene Serabyn; Michael L. Sitko; Takuya Suenaga; Hiroshi Suto; Ryuji Suzuki; Yasuhiro H. Takahashi; Michihiro Takami; Naruhisa Takato; Hiroshi Terada; Christian Thalmann; Daigo Tomono; Edwin L. Turner; Makoto Watanabe; Toru Yamada; Hideki Takami; Tomonori Usuda; Motohide Tamura

doi:10.3847/0004-637X/828/1/2

CONSTRAINING the MOVEMENT of the SPIRAL FEATURES and the LOCATIONS of PLANETARY BODIES WITHIN the AB AUR SYSTEM

Jamie R. Lomax, John P. Wisniewski, Carol A. Grady, Michael W. McElwain, Jun Hashimoto, Tomoyuki Kudo, Nobuhiko Kusakabe, Yoshiko K. Okamoto, Misato Fukagawa, Lyu Abe, Wolfgang Brandner, Timothy D. Brandt, Joseph C. Carson, Thayne M. Currie, Sebastian Egner, Markus Feldt, Miwa Goto, Olivier Guyon, Yutaka Hayano, Masahiko HayashiSaeko S. Hayashi, Thomas Henning, Klaus W. Hodapp, Akio Inoue, Miki Ishii, Masanori Iye, Markus Janson, Ryo Kandori, Gillian R. Knapp, Masayuki Kuzuhara, Jungmi Kwon, Taro Matsuo, Satoshi Mayama, Shoken Miyama, Munetake Momose, Jun Ichi Morino, Amaya Moro-Martin, Tetsuo Nishimura, Tae Soo Pyo, Glenn H. Schneider, Eugene Serabyn, Michael L. Sitko, Takuya Suenaga, Hiroshi Suto, Ryuji Suzuki, Yasuhiro H. Takahashi, Michihiro Takami, Naruhisa Takato, Hiroshi Terada, Christian Thalmann, Daigo Tomono, Edwin L. Turner, Makoto Watanabe, Toru Yamada, Hideki Takami, Tomonori Usuda, Motohide Tamura

研究成果: Article › 査読

5 被引用数 (Scopus)

抄録

We present a new analysis of multi-epoch, H-band, scattered light images of the AB Aur system. We use a Monte Carlo radiative transfer code to simultaneously model the system's spectral energy distribution (SED) and H-band polarized intensity (PI) imagery. We find that a disk-dominated model, as opposed to one that is envelope-dominated, can plausibly reproduce AB Aur's SED and near-IR imagery. This is consistent with previous modeling attempts presented in the literature and supports the idea that at least a subset of AB Aur's spirals originate within the disk. In light of this, we also analyzed the movement of spiral structures in multi-epoch H-band total light and PI imagery of the disk. We detect no significant rotation or change in spatial location of the spiral structures in these data, which span a 5.8-year baseline. If such structures are caused by disk-planet interactions, the lack of observed rotation constrains the location of the orbit of planetary perturbers to be >47 au.

本文言語	English
論文番号	2
ジャーナル	Astrophysical Journal
巻	828
号	1
DOI	https://doi.org/10.3847/0004-637X/828/1/2
出版ステータス	Published - 2016 9月 1
外部発表	はい

ASJC Scopus subject areas

天文学と天体物理学
宇宙惑星科学

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10.3847/0004-637X/828/1/2

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Lomax, J. R., Wisniewski, J. P., Grady, C. A., McElwain, M. W., Hashimoto, J., Kudo, T., Kusakabe, N., Okamoto, Y. K., Fukagawa, M., Abe, L., Brandner, W., Brandt, T. D., Carson, J. C., Currie, T. M., Egner, S., Feldt, M., Goto, M., Guyon, O., Hayano, Y., ... Tamura, M. (2016). CONSTRAINING the MOVEMENT of the SPIRAL FEATURES and the LOCATIONS of PLANETARY BODIES WITHIN the AB AUR SYSTEM. Astrophysical Journal, 828(1), 記事 2. https://doi.org/10.3847/0004-637X/828/1/2

Lomax, JR, Wisniewski, JP, Grady, CA, McElwain, MW, Hashimoto, J, Kudo, T, Kusakabe, N, Okamoto, YK, Fukagawa, M, Abe, L, Brandner, W, Brandt, TD, Carson, JC, Currie, TM, Egner, S, Feldt, M, Goto, M, Guyon, O, Hayano, Y, Hayashi, M, Hayashi, SS, Henning, T, Hodapp, KW, Inoue, A, Ishii, M, Iye, M, Janson, M, Kandori, R, Knapp, GR, Kuzuhara, M, Kwon, J, Matsuo, T, Mayama, S, Miyama, S, Momose, M, Morino, JI, Moro-Martin, A, Nishimura, T, Pyo, TS, Schneider, GH, Serabyn, E, Sitko, ML, Suenaga, T, Suto, H, Suzuki, R, Takahashi, YH, Takami, M, Takato, N, Terada, H, Thalmann, C, Tomono, D, Turner, EL, Watanabe, M, Yamada, T, Takami, H, Usuda, T & Tamura, M 2016, 'CONSTRAINING the MOVEMENT of the SPIRAL FEATURES and the LOCATIONS of PLANETARY BODIES WITHIN the AB AUR SYSTEM', Astrophysical Journal, vol. 828, no. 1, 2. https://doi.org/10.3847/0004-637X/828/1/2

@article{80ae8b459ce7445d939fc7ffce2a4a1a,

title = "CONSTRAINING the MOVEMENT of the SPIRAL FEATURES and the LOCATIONS of PLANETARY BODIES WITHIN the AB AUR SYSTEM",

abstract = "We present a new analysis of multi-epoch, H-band, scattered light images of the AB Aur system. We use a Monte Carlo radiative transfer code to simultaneously model the system's spectral energy distribution (SED) and H-band polarized intensity (PI) imagery. We find that a disk-dominated model, as opposed to one that is envelope-dominated, can plausibly reproduce AB Aur's SED and near-IR imagery. This is consistent with previous modeling attempts presented in the literature and supports the idea that at least a subset of AB Aur's spirals originate within the disk. In light of this, we also analyzed the movement of spiral structures in multi-epoch H-band total light and PI imagery of the disk. We detect no significant rotation or change in spatial location of the spiral structures in these data, which span a 5.8-year baseline. If such structures are caused by disk-planet interactions, the lack of observed rotation constrains the location of the orbit of planetary perturbers to be >47 au.",

keywords = "planet-disk interactions, planetary systems, protoplanetary disks, radiative transfer, stars: individual (AB Aur), stars: pre-main sequence",

author = "Lomax, {Jamie R.} and Wisniewski, {John P.} and Grady, {Carol A.} and McElwain, {Michael W.} and Jun Hashimoto and Tomoyuki Kudo and Nobuhiko Kusakabe and Okamoto, {Yoshiko K.} and Misato Fukagawa and Lyu Abe and Wolfgang Brandner and Brandt, {Timothy D.} and Carson, {Joseph C.} and Currie, {Thayne M.} and Sebastian Egner and Markus Feldt and Miwa Goto and Olivier Guyon and Yutaka Hayano and Masahiko Hayashi and Hayashi, {Saeko S.} and Thomas Henning and Hodapp, {Klaus W.} and Akio Inoue and Miki Ishii and Masanori Iye and Markus Janson and Ryo Kandori and Knapp, {Gillian R.} and Masayuki Kuzuhara and Jungmi Kwon and Taro Matsuo and Satoshi Mayama and Shoken Miyama and Munetake Momose and Morino, {Jun Ichi} and Amaya Moro-Martin and Tetsuo Nishimura and Pyo, {Tae Soo} and Schneider, {Glenn H.} and Eugene Serabyn and Sitko, {Michael L.} and Takuya Suenaga and Hiroshi Suto and Ryuji Suzuki and Takahashi, {Yasuhiro H.} and Michihiro Takami and Naruhisa Takato and Hiroshi Terada and Christian Thalmann and Daigo Tomono and Turner, {Edwin L.} and Makoto Watanabe and Toru Yamada and Hideki Takami and Tomonori Usuda and Motohide Tamura",

note = "Funding Information: We acknowledge support from NSF-AST 1009203 (J.C.), 1008440 (C.G.), and 1009314 (E.R., J.W., J.H.) and the NASA Origins of Solar System program under NNX13AK17G (J.W.), RTOP 12-OSS12-0045 (M.M.), and NNG13PB64P (C.G.). This work is partly supported by a Grant-in-Aid for Science Research in a Priority Area from MEXT Japan and by the Mitsubishi Foundation. Publisher Copyright: {\textcopyright} 2016. The American Astronomical Society. All rights reserved.",

year = "2016",

month = sep,

day = "1",

doi = "10.3847/0004-637X/828/1/2",

language = "English",

volume = "828",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing Ltd.",

number = "1",

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TY - JOUR

T1 - CONSTRAINING the MOVEMENT of the SPIRAL FEATURES and the LOCATIONS of PLANETARY BODIES WITHIN the AB AUR SYSTEM

AU - Lomax, Jamie R.

AU - Wisniewski, John P.

AU - Grady, Carol A.

AU - McElwain, Michael W.

AU - Hashimoto, Jun

AU - Kudo, Tomoyuki

AU - Kusakabe, Nobuhiko

AU - Okamoto, Yoshiko K.

AU - Fukagawa, Misato

AU - Abe, Lyu

AU - Brandner, Wolfgang

AU - Brandt, Timothy D.

AU - Carson, Joseph C.

AU - Currie, Thayne M.

AU - Egner, Sebastian

AU - Feldt, Markus

AU - Goto, Miwa

AU - Guyon, Olivier

AU - Hayano, Yutaka

AU - Hayashi, Masahiko

AU - Hayashi, Saeko S.

AU - Henning, Thomas

AU - Hodapp, Klaus W.

AU - Inoue, Akio

AU - Ishii, Miki

AU - Iye, Masanori

AU - Janson, Markus

AU - Kandori, Ryo

AU - Knapp, Gillian R.

AU - Kuzuhara, Masayuki

AU - Kwon, Jungmi

AU - Matsuo, Taro

AU - Mayama, Satoshi

AU - Miyama, Shoken

AU - Momose, Munetake

AU - Morino, Jun Ichi

AU - Moro-Martin, Amaya

AU - Nishimura, Tetsuo

AU - Pyo, Tae Soo

AU - Schneider, Glenn H.

AU - Serabyn, Eugene

AU - Sitko, Michael L.

AU - Suenaga, Takuya

AU - Suto, Hiroshi

AU - Suzuki, Ryuji

AU - Takahashi, Yasuhiro H.

AU - Takami, Michihiro

AU - Takato, Naruhisa

AU - Terada, Hiroshi

AU - Thalmann, Christian

AU - Tomono, Daigo

AU - Turner, Edwin L.

AU - Watanabe, Makoto

AU - Yamada, Toru

AU - Takami, Hideki

AU - Usuda, Tomonori

AU - Tamura, Motohide

N1 - Funding Information: We acknowledge support from NSF-AST 1009203 (J.C.), 1008440 (C.G.), and 1009314 (E.R., J.W., J.H.) and the NASA Origins of Solar System program under NNX13AK17G (J.W.), RTOP 12-OSS12-0045 (M.M.), and NNG13PB64P (C.G.). This work is partly supported by a Grant-in-Aid for Science Research in a Priority Area from MEXT Japan and by the Mitsubishi Foundation. Publisher Copyright: © 2016. The American Astronomical Society. All rights reserved.

PY - 2016/9/1

Y1 - 2016/9/1

N2 - We present a new analysis of multi-epoch, H-band, scattered light images of the AB Aur system. We use a Monte Carlo radiative transfer code to simultaneously model the system's spectral energy distribution (SED) and H-band polarized intensity (PI) imagery. We find that a disk-dominated model, as opposed to one that is envelope-dominated, can plausibly reproduce AB Aur's SED and near-IR imagery. This is consistent with previous modeling attempts presented in the literature and supports the idea that at least a subset of AB Aur's spirals originate within the disk. In light of this, we also analyzed the movement of spiral structures in multi-epoch H-band total light and PI imagery of the disk. We detect no significant rotation or change in spatial location of the spiral structures in these data, which span a 5.8-year baseline. If such structures are caused by disk-planet interactions, the lack of observed rotation constrains the location of the orbit of planetary perturbers to be >47 au.

AB - We present a new analysis of multi-epoch, H-band, scattered light images of the AB Aur system. We use a Monte Carlo radiative transfer code to simultaneously model the system's spectral energy distribution (SED) and H-band polarized intensity (PI) imagery. We find that a disk-dominated model, as opposed to one that is envelope-dominated, can plausibly reproduce AB Aur's SED and near-IR imagery. This is consistent with previous modeling attempts presented in the literature and supports the idea that at least a subset of AB Aur's spirals originate within the disk. In light of this, we also analyzed the movement of spiral structures in multi-epoch H-band total light and PI imagery of the disk. We detect no significant rotation or change in spatial location of the spiral structures in these data, which span a 5.8-year baseline. If such structures are caused by disk-planet interactions, the lack of observed rotation constrains the location of the orbit of planetary perturbers to be >47 au.

KW - planet-disk interactions

KW - planetary systems

KW - protoplanetary disks

KW - radiative transfer

KW - stars: individual (AB Aur)

KW - stars: pre-main sequence

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JO - Astrophysical Journal

JF - Astrophysical Journal

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ER -

CONSTRAINING the MOVEMENT of the SPIRAL FEATURES and the LOCATIONS of PLANETARY BODIES WITHIN the AB AUR SYSTEM

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