An Exo-Kuiper Belt with an Extended Halo around HD 191089 in Scattered Light

Bin Ren; Élodie Choquet; Marshall D. Perrin; Gaspard Duchěne; John H. Debes; Laurent Pueyo; Malena Rice; Christine Chen; Glenn Schneider; Thomas M. Esposito; Charles A. Poteet; Jason J. Wang; S. Mark Ammons; Megan Ansdell; Pauline Arriaga; Vanessa P. Bailey; Travis Barman; Juan Sebastián Bruzzone; Joanna Bulger; Jeffrey Chilcote; Tara Cotten; Robert J. De Rosa; Rene Doyon; Michael P. Fitzgerald; Katherine B. Follette; Stephen J. Goodsell; Benjamin L. Gerard; James R. Graham; Alexandra Z. Greenbaum; J. Brendan Hagan; Pascale Hibon; Dean C. Hines; Li Wei Hung; Patrick Ingraham; Paul Kalas; Quinn Konopacky; James E. Larkin; Bruce Macintosh; Jérôme Maire; Franck Marchis; Christian Marois; Johan Mazoyer; François Ménard; Stanimir Metchev; Maxwell A. Millar-Blanchaer; Tushar Mittal; Margaret Moerchen; Eric L. Nielsen; Mamadou N'Diaye; Rebecca Oppenheimer; David Palmer; Jennifer Patience; Christophe Pinte; Lisa Poyneer; Abhijith Rajan; Julien Rameau; Fredrik T. Rantakyrö; Jean Baptiste Ruffio; Dominic Ryan; Dmitry Savransky; Adam C. Schneider; Anand Sivaramakrishnan; Inseok Song; Rémi Soummer; Christopher Stark; Sandrine Thomas; Arthur Vigan; J. Kent Wallace; Kimberly Ward-Duong; Sloane Wiktorowicz; Schuyler Wolff; Marie Ygouf; Colin Norman

doi:10.3847/1538-4357/ab3403

An Exo-Kuiper Belt with an Extended Halo around HD 191089 in Scattered Light

Bin Ren, Élodie Choquet, Marshall D. Perrin, Gaspard Duchěne, John H. Debes, Laurent Pueyo, Malena Rice, Christine Chen, Glenn Schneider, Thomas M. Esposito, Charles A. Poteet, Jason J. Wang, S. Mark Ammons, Megan Ansdell, Pauline Arriaga, Vanessa P. Bailey, Travis Barman, Juan Sebastián Bruzzone, Joanna Bulger, Jeffrey ChilcoteTara Cotten, Robert J. De Rosa, Rene Doyon, Michael P. Fitzgerald, Katherine B. Follette, Stephen J. Goodsell, Benjamin L. Gerard, James R. Graham, Alexandra Z. Greenbaum, J. Brendan Hagan, Pascale Hibon, Dean C. Hines, Li Wei Hung, Patrick Ingraham, Paul Kalas, Quinn Konopacky, James E. Larkin, Bruce Macintosh, Jérôme Maire, Franck Marchis, Christian Marois, Johan Mazoyer, François Ménard, Stanimir Metchev, Maxwell A. Millar-Blanchaer, Tushar Mittal, Margaret Moerchen, Eric L. Nielsen, Mamadou N'Diaye, Rebecca Oppenheimer, David Palmer, Jennifer Patience, Christophe Pinte, Lisa Poyneer, Abhijith Rajan, Julien Rameau, Fredrik T. Rantakyrö, Jean Baptiste Ruffio, Dominic Ryan, Dmitry Savransky, Adam C. Schneider, Anand Sivaramakrishnan, Inseok Song, Rémi Soummer, Christopher Stark, Sandrine Thomas, Arthur Vigan, J. Kent Wallace, Kimberly Ward-Duong, Sloane Wiktorowicz, Schuyler Wolff, Marie Ygouf, Colin Norman

Earth and Space Exploration, School of (SESE)

Research output: Contribution to journal › Article › peer-review

34 Scopus citations

Abstract

We have obtained Hubble Space Telescope STIS and NICMOS and Gemini/GPI scattered-light images of the HD 191089 debris disk. We identify two spatial components: a ring resembling the Kuiper Belt in radial extent (FWHM ∼ 25 au, centered at ∼46 au) and a halo extending to ∼640 au. We find that the halo is significantly bluer than the ring, consistent with the scenario that the ring serves as the "birth ring" for the smaller dust in the halo. We measure the scattering phase functions in the 30°-150° scattering-angle range and find that the halo dust is more forward- and backward-scattering than the ring dust. We measure a surface density power-law index of -0.68 ± 0.04 for the halo, which indicates the slowdown of the radial outward motion of the dust. Using radiative transfer modeling, we attempt to simultaneously reproduce the (visible) total and (near-infrared) polarized intensity images of the birth ring. Our modeling leads to mutually inconsistent results, indicating that more complex models, such as the inclusion of more realistic aggregate particles, are needed.

Original language	English (US)
Article number	64
Journal	Astrophysical Journal
Volume	882
Issue number	1
DOIs	https://doi.org/10.3847/1538-4357/ab3403
State	Published - Sep 1 2019

Keywords

protoplanetary disks
radiative transfer
stars: imaging
stars: individual (HD 191089)
techniques: image processing

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.3847/1538-4357/ab3403

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Ren, B., Choquet, É., Perrin, M. D., Duchěne, G., Debes, J. H., Pueyo, L., Rice, M., Chen, C., Schneider, G., Esposito, T. M., Poteet, C. A., Wang, J. J., Ammons, S. M., Ansdell, M., Arriaga, P., Bailey, V. P., Barman, T., Bruzzone, J. S., Bulger, J., ... Norman, C. (2019). An Exo-Kuiper Belt with an Extended Halo around HD 191089 in Scattered Light. Astrophysical Journal, 882(1), Article 64. https://doi.org/10.3847/1538-4357/ab3403

Ren, B, Choquet, É, Perrin, MD, Duchěne, G, Debes, JH, Pueyo, L, Rice, M, Chen, C, Schneider, G, Esposito, TM, Poteet, CA, Wang, JJ, Ammons, SM, Ansdell, M, Arriaga, P, Bailey, VP, Barman, T, Bruzzone, JS, Bulger, J, Chilcote, J, Cotten, T, De Rosa, RJ, Doyon, R, Fitzgerald, MP, Follette, KB, Goodsell, SJ, Gerard, BL, Graham, JR, Greenbaum, AZ, Hagan, JB, Hibon, P, Hines, DC, Hung, LW, Ingraham, P, Kalas, P, Konopacky, Q, Larkin, JE, Macintosh, B, Maire, J, Marchis, F, Marois, C, Mazoyer, J, Ménard, F, Metchev, S, Millar-Blanchaer, MA, Mittal, T, Moerchen, M, Nielsen, EL, N'Diaye, M, Oppenheimer, R, Palmer, D, Patience, J, Pinte, C, Poyneer, L, Rajan, A, Rameau, J, Rantakyrö, FT, Ruffio, JB, Ryan, D, Savransky, D, Schneider, AC, Sivaramakrishnan, A, Song, I, Soummer, R, Stark, C, Thomas, S, Vigan, A, Wallace, JK, Ward-Duong, K, Wiktorowicz, S, Wolff, S, Ygouf, M & Norman, C 2019, 'An Exo-Kuiper Belt with an Extended Halo around HD 191089 in Scattered Light', Astrophysical Journal, vol. 882, no. 1, 64. https://doi.org/10.3847/1538-4357/ab3403

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title = "An Exo-Kuiper Belt with an Extended Halo around HD 191089 in Scattered Light",

abstract = "We have obtained Hubble Space Telescope STIS and NICMOS and Gemini/GPI scattered-light images of the HD 191089 debris disk. We identify two spatial components: a ring resembling the Kuiper Belt in radial extent (FWHM ∼ 25 au, centered at ∼46 au) and a halo extending to ∼640 au. We find that the halo is significantly bluer than the ring, consistent with the scenario that the ring serves as the {"}birth ring{"} for the smaller dust in the halo. We measure the scattering phase functions in the 30°-150° scattering-angle range and find that the halo dust is more forward- and backward-scattering than the ring dust. We measure a surface density power-law index of -0.68 ± 0.04 for the halo, which indicates the slowdown of the radial outward motion of the dust. Using radiative transfer modeling, we attempt to simultaneously reproduce the (visible) total and (near-infrared) polarized intensity images of the birth ring. Our modeling leads to mutually inconsistent results, indicating that more complex models, such as the inclusion of more realistic aggregate particles, are needed.",

keywords = "protoplanetary disks, radiative transfer, stars: imaging, stars: individual (HD 191089), techniques: image processing",

author = "Bin Ren and {\'E}lodie Choquet and Perrin, {Marshall D.} and Gaspard Duch{\v e}ne and Debes, {John H.} and Laurent Pueyo and Malena Rice and Christine Chen and Glenn Schneider and Esposito, {Thomas M.} and Poteet, {Charles A.} and Wang, {Jason J.} and Ammons, {S. Mark} and Megan Ansdell and Pauline Arriaga and Bailey, {Vanessa P.} and Travis Barman and Bruzzone, {Juan Sebasti{\'a}n} and Joanna Bulger and Jeffrey Chilcote and Tara Cotten and {De Rosa}, {Robert J.} and Rene Doyon and Fitzgerald, {Michael P.} and Follette, {Katherine B.} and Goodsell, {Stephen J.} and Gerard, {Benjamin L.} and Graham, {James R.} and Greenbaum, {Alexandra Z.} and Hagan, {J. Brendan} and Pascale Hibon and Hines, {Dean C.} and Hung, {Li Wei} and Patrick Ingraham and Paul Kalas and Quinn Konopacky and Larkin, {James E.} and Bruce Macintosh and J{\'e}r{\^o}me Maire and Franck Marchis and Christian Marois and Johan Mazoyer and Fran{\c c}ois M{\'e}nard and Stanimir Metchev and Millar-Blanchaer, {Maxwell A.} and Tushar Mittal and Margaret Moerchen and Nielsen, {Eric L.} and Mamadou N'Diaye and Rebecca Oppenheimer and David Palmer and Jennifer Patience and Christophe Pinte and Lisa Poyneer and Abhijith Rajan and Julien Rameau and Rantakyr{\"o}, {Fredrik T.} and Ruffio, {Jean Baptiste} and Dominic Ryan and Dmitry Savransky and Schneider, {Adam C.} and Anand Sivaramakrishnan and Inseok Song and R{\'e}mi Soummer and Christopher Stark and Sandrine Thomas and Arthur Vigan and Wallace, {J. Kent} and Kimberly Ward-Duong and Sloane Wiktorowicz and Schuyler Wolff and Marie Ygouf and Colin Norman",

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month = sep,

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doi = "10.3847/1538-4357/ab3403",

language = "English (US)",

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T1 - An Exo-Kuiper Belt with an Extended Halo around HD 191089 in Scattered Light

AU - Ren, Bin

AU - Choquet, Élodie

AU - Perrin, Marshall D.

AU - Duchěne, Gaspard

AU - Debes, John H.

AU - Pueyo, Laurent

AU - Rice, Malena

AU - Chen, Christine

AU - Schneider, Glenn

AU - Esposito, Thomas M.

AU - Poteet, Charles A.

AU - Wang, Jason J.

AU - Ammons, S. Mark

AU - Ansdell, Megan

AU - Arriaga, Pauline

AU - Bailey, Vanessa P.

AU - Barman, Travis

AU - Bruzzone, Juan Sebastián

AU - Bulger, Joanna

AU - Chilcote, Jeffrey

AU - Cotten, Tara

AU - De Rosa, Robert J.

AU - Doyon, Rene

AU - Fitzgerald, Michael P.

AU - Follette, Katherine B.

AU - Goodsell, Stephen J.

AU - Gerard, Benjamin L.

AU - Graham, James R.

AU - Greenbaum, Alexandra Z.

AU - Hagan, J. Brendan

AU - Hibon, Pascale

AU - Hines, Dean C.

AU - Hung, Li Wei

AU - Ingraham, Patrick

AU - Kalas, Paul

AU - Konopacky, Quinn

AU - Larkin, James E.

AU - Macintosh, Bruce

AU - Maire, Jérôme

AU - Marchis, Franck

AU - Marois, Christian

AU - Mazoyer, Johan

AU - Ménard, François

AU - Metchev, Stanimir

AU - Millar-Blanchaer, Maxwell A.

AU - Mittal, Tushar

AU - Moerchen, Margaret

AU - Nielsen, Eric L.

AU - N'Diaye, Mamadou

AU - Oppenheimer, Rebecca

AU - Palmer, David

AU - Patience, Jennifer

AU - Pinte, Christophe

AU - Poyneer, Lisa

AU - Rajan, Abhijith

AU - Rameau, Julien

AU - Rantakyrö, Fredrik T.

AU - Ruffio, Jean Baptiste

AU - Ryan, Dominic

AU - Savransky, Dmitry

AU - Schneider, Adam C.

AU - Sivaramakrishnan, Anand

AU - Song, Inseok

AU - Soummer, Rémi

AU - Stark, Christopher

AU - Thomas, Sandrine

AU - Vigan, Arthur

AU - Wallace, J. Kent

AU - Ward-Duong, Kimberly

AU - Wiktorowicz, Sloane

AU - Wolff, Schuyler

AU - Ygouf, Marie

AU - Norman, Colin

PY - 2019/9/1

Y1 - 2019/9/1

N2 - We have obtained Hubble Space Telescope STIS and NICMOS and Gemini/GPI scattered-light images of the HD 191089 debris disk. We identify two spatial components: a ring resembling the Kuiper Belt in radial extent (FWHM ∼ 25 au, centered at ∼46 au) and a halo extending to ∼640 au. We find that the halo is significantly bluer than the ring, consistent with the scenario that the ring serves as the "birth ring" for the smaller dust in the halo. We measure the scattering phase functions in the 30°-150° scattering-angle range and find that the halo dust is more forward- and backward-scattering than the ring dust. We measure a surface density power-law index of -0.68 ± 0.04 for the halo, which indicates the slowdown of the radial outward motion of the dust. Using radiative transfer modeling, we attempt to simultaneously reproduce the (visible) total and (near-infrared) polarized intensity images of the birth ring. Our modeling leads to mutually inconsistent results, indicating that more complex models, such as the inclusion of more realistic aggregate particles, are needed.

AB - We have obtained Hubble Space Telescope STIS and NICMOS and Gemini/GPI scattered-light images of the HD 191089 debris disk. We identify two spatial components: a ring resembling the Kuiper Belt in radial extent (FWHM ∼ 25 au, centered at ∼46 au) and a halo extending to ∼640 au. We find that the halo is significantly bluer than the ring, consistent with the scenario that the ring serves as the "birth ring" for the smaller dust in the halo. We measure the scattering phase functions in the 30°-150° scattering-angle range and find that the halo dust is more forward- and backward-scattering than the ring dust. We measure a surface density power-law index of -0.68 ± 0.04 for the halo, which indicates the slowdown of the radial outward motion of the dust. Using radiative transfer modeling, we attempt to simultaneously reproduce the (visible) total and (near-infrared) polarized intensity images of the birth ring. Our modeling leads to mutually inconsistent results, indicating that more complex models, such as the inclusion of more realistic aggregate particles, are needed.

KW - protoplanetary disks

KW - radiative transfer

KW - stars: imaging

KW - stars: individual (HD 191089)

KW - techniques: image processing

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DO - 10.3847/1538-4357/ab3403

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JO - Astrophysical Journal

JF - Astrophysical Journal

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ER -

An Exo-Kuiper Belt with an Extended Halo around HD 191089 in Scattered Light

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