Comprehensive Analysis of HD 105, A Young Solar System Analog

Article


Marshall, J. P., Milli, J., Choquet, E., del Burgo, C., Kennedy, G. M., Matra, L., Ertel, S. and Boccaletti, A.. 2018. "Comprehensive Analysis of HD 105, A Young Solar System Analog." The Astrophysical Journal: an international review of astronomy and astronomical physics. 869 (1), pp. 1-12. https://doi.org/10.3847/1538-4357/aaec6a
Article Title

Comprehensive Analysis of HD 105, A Young Solar System Analog

ERA Journal ID1057
Article CategoryArticle
AuthorsMarshall, J. P. (Author), Milli, J. (Author), Choquet, E. (Author), del Burgo, C. (Author), Kennedy, G. M. (Author), Matra, L. (Author), Ertel, S. (Author) and Boccaletti, A. (Author)
Journal TitleThe Astrophysical Journal: an international review of astronomy and astronomical physics
Journal Citation869 (1), pp. 1-12
Article Number10
Number of Pages12
Year2018
PublisherIOP Publishing
Place of PublicationUnited States
ISSN0004-637X
1538-4357
Digital Object Identifier (DOI)https://doi.org/10.3847/1538-4357/aaec6a
Web Address (URL)https://iopscience.iop.org/article/10.3847/1538-4357/aaec6a
Abstract

HD 105 is a nearby, pre-main-sequence G0 star hosting a moderately bright debris disk (Ldust/L⋆ ∼ 2.6 × 10−4). The star and its surroundings might therefore be considered an analog of the young solar system. We refine the stellar parameters based on an improved Gaia parallax distance and identify it as a pre-main-sequence star with an age of 50 ± 16 Myr. The circumstellar disk was marginally resolved by Herschel/PACS imaging at far-infrared wavelengths. Here, we present an archival ALMA observation at 1.3 mm, revealing the extent and orientation of the disk. We also present Hubble Space Telescope (HST)/NICMOS and VLT/SPHERE near-infrared images, where we recover the disk in scattered light at the ≥5σ level. This was achieved by employing a novel annular averaging technique and is the first time this has been achieved for a disk in scattered light. Simultaneous modeling of the available photometry, disk architecture, and detection in scattered light allow better determination of the disk's architecture, and dust grain minimum size, composition, and albedo. We measure the dust albedo to lie between 0.19 and 0.06, the lower value being consistent with Edgeworth–Kuiper Belt objects.

Keywordscircumstellar matter; planetary systems; stars: individual (HD 105)
ANZSRC Field of Research 2020519999. Other physical sciences not elsewhere classified
510109. Stellar astronomy and planetary systems
510101. Astrobiology
Byline AffiliationsComputational Engineering and Science Research Centre
European Southern Observatory, Chile
California Institute of Technology (Caltech), United States
National Institute of Astrophysics Optics and Electronics, Mexico
University of Warwick, United Kingdom
Center for Astrophysics Harvard and Smithsonian, United States
University of Arizona, United States
Laboratory of Space Science and Astrophysical Instrumentation, France
Institution of OriginUniversity of Southern Queensland
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Wyatt, M. C., Kennedy, G., Sibthorpe, B., Moro-Martin, A., Lestrade, J. -F., Ivison, R. J., Matthews, B., Udry, S., Greaves, J. S., Kalas, P., Lawler, S., Su, K. Y. L., Rieke, G. H., Booth, M., Bryden, G., Horner, J., Kavelaars, J. J. and Wilner, D.. 2012. "Herschel imaging of 61Vir: implications for the prevalence of debris in low-mass planetary systems." Monthly Notices of the Royal Astronomical Society. 424 (2), pp. 1206-1223. https://doi.org/10.1111/j.1365-2966.2012.21298.x
Revisiting the proposed planetary system orbiting the eclipsing polar HU Aquarii
Wittenmyer, Robert A., Horner, J., Marshall, J. P., Butters, O. W. and Tinney, C. G.. 2012. "Revisiting the proposed planetary system orbiting the eclipsing polar HU Aquarii." Monthly Notices of the Royal Astronomical Society. 419 (4), pp. 3258-3267. https://doi.org/10.1111/j.1365-2966.2011.19966.x
Dynamical simulations of the HR8799 planetary system
Marshall, J., Horner, J. and Carter, A.. 2010. "Dynamical simulations of the HR8799 planetary system ." 4th Biennial Astrobiology Society of Britain Conference (ASB4): Building Habitable Worlds . London, United Kingdom 07 - 09 Apr 2010 Cambridge, United Kingdom. https://doi.org/10.1017/S1473550410000297
On the dynamical stability of the proposed planetary system orbiting NSVS 14256825
Wittenmyer, Robert A., Horner, J. and Marshall, J. P.. 2013. "On the dynamical stability of the proposed planetary system orbiting NSVS 14256825." Monthly Notices of the Royal Astronomical Society. 431 (3), pp. 2150-2154. https://doi.org/10.1093/mnras/stt299
Main-sequence progenitor configurations of the NN ser candidate circumbinary planetary system are dynamically unstable
Mustill, Alexander J., Marshall, Jonathan P., Villaver, Eva, Veras, Dimitri, Davis, Philip J., Horner, Jonathan and Wittenmyer, Robert A.. 2013. "Main-sequence progenitor configurations of the NN ser candidate circumbinary planetary system are dynamically unstable." Monthly Notices of the Royal Astronomical Society. 436 (3), pp. 2515-2521. https://doi.org/10.1093/mnras/stt1754
A dynamical analysis of the proposed circumbinary HWVirginis planetary system
Horner, J., Hinse, T. C., Wittenmyer, R. A., Marshall, J. P. and Tinney, C. G.. 2012. "A dynamical analysis of the proposed circumbinary HWVirginis planetary system." Monthly Notices of the Royal Astronomical Society. 427 (4), pp. 2812-2823. https://doi.org/10.1111/j.1365-2966.2012.22046.x
A detailed dynamical investigation of the proposed QS Virginis planetary system
Horner, J., Wittenmyer, R. A., Hinse, T. C., Marshall, J. P., Mustill, A. J. and Tinney, C. G.. 2013. "A detailed dynamical investigation of the proposed QS Virginis planetary system." Monthly Notices of the Royal Astronomical Society. 435 (3), pp. 2033-2039. https://doi.org/10.1093/mnras/stt1420
Evolution from protoplanetary to debris discs: the transition disc around HD 166191
Kennedy, G. M., Murphy, S. J., Lisse, C. M., Menard, F., Sitko, M. L., Wyatt, M. C., Bayliss, D. D. R., DeMeo, F. E., Crawford, K. B., Kim, D. L., Rudy, R. J., Russell, R. W., Sibthorpe, B., Skinner, M. A. and Zhou, G.. 2014. "Evolution from protoplanetary to debris discs: the transition disc around HD 166191." Monthly Notices of the Royal Astronomical Society. 438 (4), pp. 3299-3309. https://doi.org/10.1093/mnras/stt2435