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Warm Debris Disks with WISE and HST

Published online by Cambridge University Press:  27 January 2016

Deborah Padgett  and
Karl Stapelfeldt
Deborah Padgett
Affiliation:
Code 665, NASA Goddard Space Flight Center email: [email protected]
Karl Stapelfeldt
Affiliation:
Code 667, NASA Goddard Space Flight Center email: [email protected]
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Abstract

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Using 22 μm data from the Wide Field Infrared Survey Explorer (WISE), we have completed a sensitive all-sky survey for debris disks in Hipparcos and Tycho catalog stars within 120 pc. This warm excess emission traces material in the circumstellar region likely to host terrestrial planets. Several hundred previously unknown debris disk candidates were identified. We are currently performing follow-up observations to characterize the stars, companions, and circumstellar material in these systems with a variety of facilities including Keck, Herschel, and HST. Thirteen WISE debris disks have been observed to date using HST/STIS coronagraphy. Five of these disks have been detected in scattered light. One is a large and highly asymmetric edge-on disk which appears to be both warped and bifurcated.

Keywords

stars: circumstellar matterstars: planetary systemsprotoplanetary disks
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S314: Young Stars & Planets Near the Sun , November 2015 , pp. 175 - 178
Copyright
Copyright © International Astronomical Union 2016 

References

Acke, B., Min, M., Dominik, C., Vandenbussche, B., Sibthorpe, B., Waelkens, C., Olofsson, G., Degroote, P., Smolders, K., & Pantin, E., et al. 2012, A&A, 540, 125Google Scholar
Booth, M., Kennedy, G., Sibthorpe, B., Matthews, B. C., Wyatt, M. C., Duchene, G., Kavelaars, J. J., Rodriguez, D., Greave, J. S., Koning, A.et al. 2013, MNRAS, 428, 1263Google Scholar
Carpenter, J. M., Mamajek, E. E., Hillenbrand, L. A., & Meyer, M. R. 2009, ApJ, 705, 1646CrossRefGoogle Scholar
Chiang, E., Kite, E., Graham, J. R., & Clampin, M. 2009, ApJ, 693, 734CrossRefGoogle Scholar
Dermott, S. F., Jayaraman, S., Xu, Y. L., Gustarfson, B. A. S.., & Liou, J. C. 1994, Nature, 369, 719CrossRefGoogle Scholar
Hinkley, S., Mawet, D., Stapelfeldt, K., Padgett, D., Morales, F., & Serabyn, E. 2014, Proceedings of the conference Thirty years of beta Pic and debris disks studies, Lagrange, A.-M. & Boccaletti, A., eds., p.40Google Scholar
Kalas, P., Graham, J. R., & Clampin, M. 2005, Nature, 435, 1067Google Scholar
Kalas, P., Graham, J., Chiang, E., Fitzgerald, M., Clampin, M., Kite, E., Stapelfeldt, K., Marois, C., & Krist, J. 2008, Science, 322, 1345Google Scholar
Kalas, P., Graham, J. R., Fitzgerald, M. P., & Clampin, M. 2013, ApJ, 775, 56CrossRefGoogle Scholar
Krist, J. E., Stapelfeldt, K. R., Bryden, G., & Plavchan, P. 2012, AJ, 144, 45CrossRefGoogle Scholar
Lagrange, A.-M., Bonnefoy, M., Chauvin, G., Apai, D., Ehrenreich, D., Boccaletti, A., Gratadour, D., Rouan, D., Mouillet, D., Lacour, S., & Kaspar, M. 2010, Science, 329, 57Google Scholar
Lohne, T., Eiroa, C., Augereau, J.-C., Ertel, S., Marshall, J. P., Mora, A., Absil, O., Stapelfeldt, K., Thebault, P., Bayo, A., et al. 2012, Astronomische Nachrichten, 333, 441Google Scholar
Marois, C., Macintosh, B., Barman, T., Zuckerman, B., Song, I., Patience, J., Lafreniere, D., & Doyon, R. 2008, Science, 322, 1348Google Scholar
Marois, C., Zuckerman, B., Konopacky, Q. M., Macintosh, B., & Barman, T. 2010, Nature, 468, 1080Google Scholar
Matthews, B. C., Sibthorpe, B., Kennedy, G., Phillips, N., Churcher, L., Duchene, G., Greaves, J. S., Lestrade, J.-F., Moro-Martin, A., & Wyatt, M. C., et al. 2010, A&A, 518, 135Google Scholar
McDonald, I., Zijlstra, A., & Boyer, M. 2012, MNRAS, 427, 343CrossRefGoogle Scholar
Patel, R., Metchev, S., & Heinze, A. 2014, ApJS, 212, 10Google Scholar
Quillen, A. C. 2006, MNRAS, 372, 14Google Scholar
Rameau, J., Chauvin, G., Lagrange, A.-M., Meshkat, T., Boccaletti, A., Quanz, S. P., Currie, T., Mawet, D., Girard, J. H., Bonnefoy, M., & Kenworthy, M. 2013, ApJ, 779, 26Google Scholar
Rieke, G. H., Su, K. Y. L., Stansberry, J. A., Trilling, D., Bryden, G., Muzerolle, J., White, B., Gorlova, N., Young, E. T., Beichman, C. A., Stapelfeldt, K. R., & Hines, D. C. 2005, ApJ, 620, 1010Google Scholar
Rodigas, T. J., Malhotra, R., & Hinz, P. M. 2014, ApJ, 780, 65CrossRefGoogle Scholar
Smith, B. & Terrile, R. 1984, Science, 226, 1421Google Scholar
Su, K. Y. L., Rieke, G. H., Stapelfeldt, K. R., Malhotra, R., Bryden, G., Smith, P. S., Misselt, K. A., Moro-Martin, A., & Williams, J. P. 2009, ApJ, 705, 314Google Scholar
Wright, E. L., Eisenhardt, P. R. M., Mainzer, A. K., Ressler, M. E., Cutri, R. M., Jarrett, T., Kirkpatrick, J. D., Padgett, D., McMillan, R. S., Skrutskie, M.et al. 2010, AJ, 140, 1868Google Scholar
Wyatt, M. 2008, ARAA, 46, 339Google Scholar