Gemini Planet Imager Spectroscopy of the Dusty Substellar Companion HD 206893 B
Abstract
In this paper, we present new near-infrared Gemini Planet Imager (GPI) spectroscopy of HD 206893 B, a substellar companion orbiting within the debris disk of its F5V star. The J, H, K1, and K2 spectra from GPI demonstrate the extraordinarily red colors of the object, confirming it as the reddest substellar object observed to date. The significant flux increase throughout the infrared presents a challenging atmosphere to model with existing grids. Best-fit values vary from 1200 to 1800 K for effective temperature and from 3.0 to 5.0 for log(g), depending on which individual wavelength band is fit and which model suite is applied. The extreme redness of the companion can be partially reconciled by invoking a high-altitude layer of submicron dust particles, similar to dereddening approaches applied to the peculiar red field L dwarf population. However, reconciling the HD 206893 B spectra with even those of the reddest low-gravity L dwarf spectra still requires the contribution of additional atmospheric dust, potentially due to the debris disk environment in which the companion resides. Orbit fitting from 4 yr of astrometric monitoring is consistent with a ~30 yr period, an orbital inclination of 147°, and a semimajor axis of 10 au, wellmore »
- Authors:
-
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- Amherst College, MA (United States); Arizona State Univ., Tempe, AZ (United States)
- Arizona State Univ., Tempe, AZ (United States)
- Amherst College, MA (United States)
- Stanford Univ., CA (United States); European Southern Observatory, Santiago (Chile)
- Univ. Grenoble Alpes (France); Centre National de la Recherche Scientifique (CNRS), Grenoble (France); Univ. of Montreal, QC (Canada)
- NASA Ames Research Center (ARC), Mountain View, CA (United States)
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Stanford Univ., CA (United States)
- Space Telescope Science Inst., Baltimore, MD (United States)
- Univ. of Michigan, Ann Arbor, MI (United States)
- Univ. of Georgia, Athens, GA (United States)
- California Inst. of Technology (CalTech), Pasadena, CA (United States); Univ. of California, Berkeley, CA (United States)
- Stanford Univ., CA (United States); Univ. of California, Berkeley, CA (United States)
- Univ. Grenoble Alpes (France); Univ. of California, Berkeley, CA (United States)
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- California Inst. of Technology (CalTech), Pasadena, CA (United States)
- Univ. of Arizona, Tucson, AZ (United States)
- Univ. of Hawaii, Honolulu, HI (United States); National Astronomical Observatory of Japan (NAOJ), Hilo, HI (United States)
- Stanford Univ., CA (United States); Univ. of Notre Dame, IN (United States)
- Univ. of Montreal, QC (Canada)
- Univ. of California, Berkeley, CA (United States)
- Univ. of California, Los Angeles, CA (United States)
- Univ. of California, Santa Cruz, CA (United States); National Research Council of Canada, Ottawa, ON (Canada)
- Gemini Observatory, Hilo, HI (United States)
- European Southern Observatory, Santiago (Chile)
- National Park Service, Fort Collins, CO (United States)
- Large Synoptic Survey Telescope, Tucson, AZ (United States)
- Univ. of California, Berkeley, CA (United States); SETI Inst., Mountain View, CA (United States)
- Univ. of California San Diego, La Jolla, CA (United States)
- SETI Inst., Mountain View, CA (United States)
- National Research Council of Canada, Ottawa, ON (Canada); Univ. of Victoria, BC (Canada)
- Univ. of Western Ontario, London, ON (Canada); Stony Brook Univ., NY (United States)
- American Museum of Natural History (AMNH), New York, NY (United States)
- Gemini Observatory, La Serena (Chile)
- Johns Hopkins Univ., Baltimore, MD (United States)
- Cornell Univ., Ithaca, NY (United States)
- US Naval Observatory, Flagstaff Station, Flagstaff, AZ (United States); George Mason Univ., Fairfax, VA (United States)
- The Aerospace Corporation, El Segundo, CA (United States)
- Leiden Univ. (Netherlands)
- Publication Date:
- Research Org.:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC); Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
- Sponsoring Org.:
- National Science Foundation (NSF); National Research Council Canada (NRC); Comisión Nacional de Investigación Científica y Tecnológica (CONICYT); Ministerio de Ciencia, Tecnologia e Innovacion Productiva (MINCYT); Ministerio da Ciencia, Tecnologia e Inovacao (MCTI); National Aeronautics and Space Administration (NASA); National Radio Astronomy Observatory (NRAO); Fonds de Recherche du Quebec; Heising-Simons Foundation; USDOE Office of Science (SC)
- OSTI Identifier:
- 1760567
- Alternate Identifier(s):
- OSTI ID: 1836923
- Report Number(s):
- LA-UR-19-29876; LLNL-JRNL-829711
Journal ID: ISSN 1538-3881; TRN: US2205748
- Grant/Contract Number:
- 89233218CNA000001; AC02-05CH11231; ACI-1548562; AST-1411868; AST-141378; AST-1518332; NNX14AJ80G; NNX15AC89G; NNX15AD95G; NN15AB52l; NNX16AD44G; SOSPA3-007; NNH15AZ59I; 51378.01-A; NAS5-26555; AC52-07NA27344
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astronomical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astronomical Journal (Online); Journal Volume: 161; Journal Issue: 1; Journal ID: ISSN 1538-3881
- Publisher:
- IOP Publishing - AAAS
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Substellar companion stars; Brown dwarfs; Debris disks; Exoplanet atmospheric composition; Orbit determination
Citation Formats
Ward-Duong, K., Patience, J., Follette, K., Rosa, R. De, Rameau, J., Marley, M., Saumon, Didier, Nielsen, E. L., Rajan, A., Greenbaum, A. Z., Lee, J., Wang, J. J., Czekala, I., Duchêne, G., Macintosh, B., Ammons, S. Mark, Bailey, V. P., Barman, T., Bulger, J., Chen, C., Chilcote, J., Cotten, T., Doyon, R., Esposito, T. M., Fitzgerald, M. P., Gerard, B. L., Goodsell, S. J., Graham, J. R., Hibon, P., Hom, J., Hung, L.-W., Ingraham, P., Kalas, P., Konopacky, Q., Larkin, J. E., Maire, J., Marchis, F., Marois, C., Metchev, S., Millar-Blanchaer, M. A., Oppenheimer, R., Palmer, D., Perrin, M., Poyneer, L., Pueyo, L., Rantakyrö, F. T., Ren, B., Ruffio, J.-B., Savransky, D., Schneider, A. C., Sivaramakrishnan, A., Song, I., Soummer, R., Tallis, M., Thomas, S., Wallace, J. Kent, Wiktorowicz, S., and Wolff, S. Gemini Planet Imager Spectroscopy of the Dusty Substellar Companion HD 206893 B. United States: N. p., 2020.
Web. doi:10.3847/1538-3881/abc263.
Ward-Duong, K., Patience, J., Follette, K., Rosa, R. De, Rameau, J., Marley, M., Saumon, Didier, Nielsen, E. L., Rajan, A., Greenbaum, A. Z., Lee, J., Wang, J. J., Czekala, I., Duchêne, G., Macintosh, B., Ammons, S. Mark, Bailey, V. P., Barman, T., Bulger, J., Chen, C., Chilcote, J., Cotten, T., Doyon, R., Esposito, T. M., Fitzgerald, M. P., Gerard, B. L., Goodsell, S. J., Graham, J. R., Hibon, P., Hom, J., Hung, L.-W., Ingraham, P., Kalas, P., Konopacky, Q., Larkin, J. E., Maire, J., Marchis, F., Marois, C., Metchev, S., Millar-Blanchaer, M. A., Oppenheimer, R., Palmer, D., Perrin, M., Poyneer, L., Pueyo, L., Rantakyrö, F. T., Ren, B., Ruffio, J.-B., Savransky, D., Schneider, A. C., Sivaramakrishnan, A., Song, I., Soummer, R., Tallis, M., Thomas, S., Wallace, J. Kent, Wiktorowicz, S., & Wolff, S. Gemini Planet Imager Spectroscopy of the Dusty Substellar Companion HD 206893 B. United States. https://doi.org/10.3847/1538-3881/abc263
Ward-Duong, K., Patience, J., Follette, K., Rosa, R. De, Rameau, J., Marley, M., Saumon, Didier, Nielsen, E. L., Rajan, A., Greenbaum, A. Z., Lee, J., Wang, J. J., Czekala, I., Duchêne, G., Macintosh, B., Ammons, S. Mark, Bailey, V. P., Barman, T., Bulger, J., Chen, C., Chilcote, J., Cotten, T., Doyon, R., Esposito, T. M., Fitzgerald, M. P., Gerard, B. L., Goodsell, S. J., Graham, J. R., Hibon, P., Hom, J., Hung, L.-W., Ingraham, P., Kalas, P., Konopacky, Q., Larkin, J. E., Maire, J., Marchis, F., Marois, C., Metchev, S., Millar-Blanchaer, M. A., Oppenheimer, R., Palmer, D., Perrin, M., Poyneer, L., Pueyo, L., Rantakyrö, F. T., Ren, B., Ruffio, J.-B., Savransky, D., Schneider, A. C., Sivaramakrishnan, A., Song, I., Soummer, R., Tallis, M., Thomas, S., Wallace, J. Kent, Wiktorowicz, S., and Wolff, S. Wed .
"Gemini Planet Imager Spectroscopy of the Dusty Substellar Companion HD 206893 B". United States. https://doi.org/10.3847/1538-3881/abc263. https://www.osti.gov/servlets/purl/1760567.
@article{osti_1760567,
title = {Gemini Planet Imager Spectroscopy of the Dusty Substellar Companion HD 206893 B},
author = {Ward-Duong, K. and Patience, J. and Follette, K. and Rosa, R. De and Rameau, J. and Marley, M. and Saumon, Didier and Nielsen, E. L. and Rajan, A. and Greenbaum, A. Z. and Lee, J. and Wang, J. J. and Czekala, I. and Duchêne, G. and Macintosh, B. and Ammons, S. Mark and Bailey, V. P. and Barman, T. and Bulger, J. and Chen, C. and Chilcote, J. and Cotten, T. and Doyon, R. and Esposito, T. M. and Fitzgerald, M. P. and Gerard, B. L. and Goodsell, S. J. and Graham, J. R. and Hibon, P. and Hom, J. and Hung, L.-W. and Ingraham, P. and Kalas, P. and Konopacky, Q. and Larkin, J. E. and Maire, J. and Marchis, F. and Marois, C. and Metchev, S. and Millar-Blanchaer, M. A. and Oppenheimer, R. and Palmer, D. and Perrin, M. and Poyneer, L. and Pueyo, L. and Rantakyrö, F. T. and Ren, B. and Ruffio, J.-B. and Savransky, D. and Schneider, A. C. and Sivaramakrishnan, A. and Song, I. and Soummer, R. and Tallis, M. and Thomas, S. and Wallace, J. Kent and Wiktorowicz, S. and Wolff, S.},
abstractNote = {In this paper, we present new near-infrared Gemini Planet Imager (GPI) spectroscopy of HD 206893 B, a substellar companion orbiting within the debris disk of its F5V star. The J, H, K1, and K2 spectra from GPI demonstrate the extraordinarily red colors of the object, confirming it as the reddest substellar object observed to date. The significant flux increase throughout the infrared presents a challenging atmosphere to model with existing grids. Best-fit values vary from 1200 to 1800 K for effective temperature and from 3.0 to 5.0 for log(g), depending on which individual wavelength band is fit and which model suite is applied. The extreme redness of the companion can be partially reconciled by invoking a high-altitude layer of submicron dust particles, similar to dereddening approaches applied to the peculiar red field L dwarf population. However, reconciling the HD 206893 B spectra with even those of the reddest low-gravity L dwarf spectra still requires the contribution of additional atmospheric dust, potentially due to the debris disk environment in which the companion resides. Orbit fitting from 4 yr of astrometric monitoring is consistent with a ~30 yr period, an orbital inclination of 147°, and a semimajor axis of 10 au, well within the estimated disk inner radius of ~50 au. As one of a very few substellar companions imaged interior to a circumstellar disk, the properties of this system offer important dynamical constraints on companion–disk interaction and provide a benchmark for substellar and planetary atmospheric study.},
doi = {10.3847/1538-3881/abc263},
journal = {The Astronomical Journal (Online)},
number = 1,
volume = 161,
place = {United States},
year = {Wed Dec 02 00:00:00 EST 2020},
month = {Wed Dec 02 00:00:00 EST 2020}
}
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