Newly seen debris disks from the HST NICMOS archive

Marshall D. Perrin; Elodie Choquet; Christine Chen; John Debes; David Golimowski; J. Brendan Hagan; Dean C. Hines; Tushar Mittal; Margaret Moerchen; Mamadou N'Diaye; Laurent Pueyo; I. Neill Reid; Glenn Schneider; Schuyler Wolff; Remi Soummer

doi:10.1017/S1743921313008922

Newly seen debris disks from the HST NICMOS archive

Marshall D. Perrin
, Elodie Choquet
, Christine Chen
, John Debes
, David Golimowski
, J. Brendan Hagan
, Dean C. Hines
, Tushar Mittal
, Margaret Moerchen
, Mamadou N'Diaye
, Laurent Pueyo
, I. Neill Reid
, Glenn Schneider
, Schuyler Wolff
, Remi Soummer

Geosciences

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

By reprocessing the NICMOS coronagraphic archive using improved PSF subtraction methods, we have obtained new images of 5 debris disks, all previously unseen using classical PSF subtractions. Three of the disks are edge on and two appear to be ring like, one of which is extremely asymmetric. Their stellar hosts are nearby, young F and G type stars (40-90 pc, 12-30 Myr), including one that is a close analog to the young sun at roughly the age at which terrestrial planets were assembling. This is a 25% increase in the sample of debris disks seen in scattered light. Analysis and modeling of the disk geometries is in process. Given these systems' youth, proximity, and brightness (V = 7.2 to 8.5), these will be superb targets for investigating planet formation, and are perfect targets for studies with GPI, SPHERE and JWST.

Original language	English (US)
Title of host publication	Exploring the Formation and Evolution of Planetary Systems
Publisher	Cambridge University Press
Pages	354-355
Number of pages	2
Edition	S299
ISBN (Print)	9781107045200
DOIs	https://doi.org/10.1017/S1743921313008922
State	Published - Jun 2013

Publication series

Name	Proceedings of the International Astronomical Union
Number	S299
Volume	8
ISSN (Print)	1743-9213
ISSN (Electronic)	1743-9221

UN SDGs

This output contributes to the following UN Sustainable Development Goals (SDGs)

SDG 3 Good Health and Well-being

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1017/S1743921313008922

Cite this

Perrin, M. D., Choquet, E., Chen, C., Debes, J., Golimowski, D., Brendan Hagan, J., Hines, D. C., Mittal, T., Moerchen, M., N'Diaye, M., Pueyo, L., Neill Reid, I., Schneider, G., Wolff, S., & Soummer, R. (2013). Newly seen debris disks from the HST NICMOS archive. In Exploring the Formation and Evolution of Planetary Systems (S299 ed., pp. 354-355). (Proceedings of the International Astronomical Union; Vol. 8, No. S299). Cambridge University Press. https://doi.org/10.1017/S1743921313008922

@inproceedings{d447a9c03d29462ca4d475aaf2fc65ef,

title = "Newly seen debris disks from the HST NICMOS archive",

abstract = "By reprocessing the NICMOS coronagraphic archive using improved PSF subtraction methods, we have obtained new images of 5 debris disks, all previously unseen using classical PSF subtractions. Three of the disks are edge on and two appear to be ring like, one of which is extremely asymmetric. Their stellar hosts are nearby, young F and G type stars (40-90 pc, 12-30 Myr), including one that is a close analog to the young sun at roughly the age at which terrestrial planets were assembling. This is a 25\% increase in the sample of debris disks seen in scattered light. Analysis and modeling of the disk geometries is in process. Given these systems' youth, proximity, and brightness (V = 7.2 to 8.5), these will be superb targets for investigating planet formation, and are perfect targets for studies with GPI, SPHERE and JWST.",

author = "Perrin, \{Marshall D.\} and Elodie Choquet and Christine Chen and John Debes and David Golimowski and \{Brendan Hagan\}, J. and Hines, \{Dean C.\} and Tushar Mittal and Margaret Moerchen and Mamadou N'Diaye and Laurent Pueyo and \{Neill Reid\}, I. and Glenn Schneider and Schuyler Wolff and Remi Soummer",

year = "2013",

month = jun,

doi = "10.1017/S1743921313008922",

language = "English (US)",

isbn = "9781107045200",

series = "Proceedings of the International Astronomical Union",

publisher = "Cambridge University Press",

number = "S299",

pages = "354--355",

booktitle = "Exploring the Formation and Evolution of Planetary Systems",

address = "United Kingdom",

edition = "S299",

}

Perrin, MD, Choquet, E, Chen, C, Debes, J, Golimowski, D, Brendan Hagan, J, Hines, DC, Mittal, T, Moerchen, M, N'Diaye, M, Pueyo, L, Neill Reid, I, Schneider, G, Wolff, S & Soummer, R 2013, Newly seen debris disks from the HST NICMOS archive. in Exploring the Formation and Evolution of Planetary Systems. S299 edn, Proceedings of the International Astronomical Union, no. S299, vol. 8, Cambridge University Press, pp. 354-355. https://doi.org/10.1017/S1743921313008922

Newly seen debris disks from the HST NICMOS archive. / Perrin, Marshall D.; Choquet, Elodie; Chen, Christine et al.
Exploring the Formation and Evolution of Planetary Systems. S299. ed. Cambridge University Press, 2013. p. 354-355 (Proceedings of the International Astronomical Union; Vol. 8, No. S299).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - Newly seen debris disks from the HST NICMOS archive

AU - Perrin, Marshall D.

AU - Choquet, Elodie

AU - Chen, Christine

AU - Debes, John

AU - Golimowski, David

AU - Brendan Hagan, J.

AU - Hines, Dean C.

AU - Mittal, Tushar

AU - Moerchen, Margaret

AU - N'Diaye, Mamadou

AU - Pueyo, Laurent

AU - Neill Reid, I.

AU - Schneider, Glenn

AU - Wolff, Schuyler

AU - Soummer, Remi

PY - 2013/6

Y1 - 2013/6

N2 - By reprocessing the NICMOS coronagraphic archive using improved PSF subtraction methods, we have obtained new images of 5 debris disks, all previously unseen using classical PSF subtractions. Three of the disks are edge on and two appear to be ring like, one of which is extremely asymmetric. Their stellar hosts are nearby, young F and G type stars (40-90 pc, 12-30 Myr), including one that is a close analog to the young sun at roughly the age at which terrestrial planets were assembling. This is a 25% increase in the sample of debris disks seen in scattered light. Analysis and modeling of the disk geometries is in process. Given these systems' youth, proximity, and brightness (V = 7.2 to 8.5), these will be superb targets for investigating planet formation, and are perfect targets for studies with GPI, SPHERE and JWST.

AB - By reprocessing the NICMOS coronagraphic archive using improved PSF subtraction methods, we have obtained new images of 5 debris disks, all previously unseen using classical PSF subtractions. Three of the disks are edge on and two appear to be ring like, one of which is extremely asymmetric. Their stellar hosts are nearby, young F and G type stars (40-90 pc, 12-30 Myr), including one that is a close analog to the young sun at roughly the age at which terrestrial planets were assembling. This is a 25% increase in the sample of debris disks seen in scattered light. Analysis and modeling of the disk geometries is in process. Given these systems' youth, proximity, and brightness (V = 7.2 to 8.5), these will be superb targets for investigating planet formation, and are perfect targets for studies with GPI, SPHERE and JWST.

UR - https://www.scopus.com/pages/publications/84891874960

UR - https://www.scopus.com/pages/publications/84891874960#tab=citedBy

U2 - 10.1017/S1743921313008922

DO - 10.1017/S1743921313008922

M3 - Conference contribution

AN - SCOPUS:84891874960

SN - 9781107045200

T3 - Proceedings of the International Astronomical Union

SP - 354

EP - 355

BT - Exploring the Formation and Evolution of Planetary Systems

PB - Cambridge University Press

ER -

Newly seen debris disks from the HST NICMOS archive

Abstract

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UN SDGs

All Science Journal Classification (ASJC) codes

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