Constraints on HD 113337 fundamental parameters and planetary system. Combining long-base visible interferometry, disc imaging, and high-contrast imaging
techniques: interferometric; techniques: high angular resolution; stars: individual: HD 113337; planetary systems; stars: fundamental parameters
Abstract :
[en] Context. HD 113337 is a main-sequence F6V field star more massive than the Sun. This star hosts one confirmed giant planet and possibly a second candidate, detected by radial velocities (RVs). The star also hosts a cold debris disc detected through the presence of an infrared excess, making it an interesting system to explore. <BR /> Aims: We aim to bring new constraints on the star's fundamental parameters, debris disc properties, and planetary companion(s) by combining complementary techniques. <BR /> Methods: We used the VEGA interferometer on the CHARA array to measure the angular diameter of HD 113337. We derived its linear radius using the parallax from the Gaia Second Data Release. We computed the bolometric flux to derive its effective temperature and luminosity, and we estimated its mass and age using evolutionary tracks. Then, we used Herschel images to partially resolve the outer debris disc and estimate its extension and inclination. Next, we acquired high-contrast images of HD 113337 with the LBTI to probe the 10-80 au separation range. Finally, we combined the deduced contrast maps with previous RVs of the star using the MESS2 software to bring upper mass limits on possible companions at all separations up to 80 au. We took advantage of the constraints on the age and inclination brought by fundamental parameter analysis and disc imaging, respectively, for this analysis. <BR /> Results: We derive a limb-darkened angular diameter of 0.386 ± 0.009 mas that converts into a linear radius of 1.50 ± 0.04 R[SUB]⊙[/SUB] for HD 113337. The fundamental parameter analysis leads to an effective temperature of 6774 ± 125 K and to two possible age solutions: one young within 14-21 Myr and one old within 0.8-1.7 Gyr. We partially resolve the known outer debris disc and model its emission. Our best solution corresponds to a radius of 85 ± 20 au, an extension of 30 ± 20 au, and an inclination within 10-30° for the outer disc. The combination of imaging contrast limits, published RV, and age and inclination solutions allows us to derive a first possible estimation of the true masses of the planetary companions: 7[SUB]-2[/SUB][SUP]+4[/SUP] M[SUB]Jup[/SUB] for HD 113337 b (confirmed companion) and 16[SUB]-3[/SUB][SUP]+10[/SUP] M[SUB]Jup[/SUB] for HD 113337 c (candidate companion). We also constrain possible additional companions at larger separations. Partly based on observations made with the VEGA/CHARA spectro-interferometer.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Borgniet, S.; LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, 92195, Meudon, France ; Université Grenoble Alpes, IPAG, CNRS, 38000, Grenoble, France
Perraut, K.; Université Grenoble Alpes, IPAG, CNRS, 38000, Grenoble, France
Su, K.; Steward Observatory, University of Arizona, 933 N Cherry Ave, Tucson, AZ, 85721, USA
Bonnefoy, M.; Université Grenoble Alpes, IPAG, CNRS, 38000, Grenoble, France ; Max Planck Institute for Astronomy, Koenigstuhl 17, 69117, Heidelberg, Germany
Delorme, P.; Université Grenoble Alpes, IPAG, CNRS, 38000, Grenoble, France
Lagrange, A.-M.; Université Grenoble Alpes, IPAG, CNRS, 38000, Grenoble, France
Bailey, V.; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
Buenzli, E.; Max Planck Institute for Astronomy, Koenigstuhl 17, 69117, Heidelberg, Germany
Defrere, Denis ; Université de Liège - ULiège > CSL (Centre Spatial de Liège)
Henning, T.; Max Planck Institute for Astronomy, Koenigstuhl 17, 69117, Heidelberg, Germany
Hinz, P.; Steward Observatory, University of Arizona, 933 N Cherry Ave, Tucson, AZ, 85721, USA
Leisenring, J.; Steward Observatory, University of Arizona, 933 N Cherry Ave, Tucson, AZ, 85721, USA
Meunier, N.; Université Grenoble Alpes, IPAG, CNRS, 38000, Grenoble, France
Constraints on HD 113337 fundamental parameters and planetary system. Combining long-base visible interferometry, disc imaging, and high-contrast imaging
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Bibliography
Allende Prieto, C., & Lambert, D. L. 1999, VizieR Online Data Catalog: 335
Bailer-Jones, C. A. L., Rybizki, J., Fouesneau, M., Mantelet, G., & Andrae, R. 2018, AJ, 156, 58
Balog, Z., Müller, T., Nielbock, M., et al. 2014, Exp. Astron., 37, 129
Baraffe, I., Chabrier, G., Barman, T. S., Allard, F., & Hauschildt, P. H. 2003, A&A, 402, 701
Boesgaard, A. M., & Tripicco, M. J. 1986, ApJ, 303, 724
Bonneau, D., Clausse, J.-M., Delfosse, X., et al. 2006, A&A, 456, 789
Bonnefoy, M., Marleau, G.-D., Galicher, R., et al. 2014a, A&A, 567, L9
Bonnefoy, M., Currie, T., Marleau, G.-D., et al. 2014b, A&A, 562, A111
Bonnefoy, M., Perraut, K., Lagrange, A.-M., et al. 2018, A&A, 618, A63
Borgniet, S., Boisse, I., Lagrange, A.-M., et al. 2014, A&A, 561, A65
Bouchy, F., Ségransan, D., Díaz, R. F., et al. 2016, A&A, 585, A46
Bourges, L., Mella, G., Lafrasse, S., et al. 2017, VizieR Online Data Catalog: II/346
Boyajian, T., von Braun, K., Feiden, G. A., et al. 2015, MNRAS, 447, 846
Casagrande, L., Schoenrich, R., Asplund, M., et al. 2011, VizieR Online Data Catalog: 353
Chauvin, G., Gratton, R., Bonnefoy, M., et al. 2018, A&A, 617, A76
Chen, C. H., Mittal, T., Kuchner, M., et al. 2014, ApJS, 211, 25
Claret, A., & Bloemen, S. 2011, VizieR Online Data Catalog: J/A+A/352/075
Cohen, M., Wheaton, W. A., & Megeath, S. T. 2003, AJ, 126, 1090
Creevey, O. L., Monteiro, M. J. P. F. G., Metcalfe, T. S., et al. 2007, ApJ, 659, 616
Crida, A., Ligi, R., Dorn, C., & Lebreton, Y. 2018, ApJ, 860, 122
Cutri, R. M., Skrutskie, M. F., Stiening, R. R. M., et al. 2014, VizieR Online Data Catalog: II/328
David, T. J., & Hillenbrand, L. A. 2015, ApJ, 804, 146
D'Orazi, V., Desidera, S., Gratton, R. G., et al. 2017, A&A, 598, A19
ESA, 1997, The HIPPARCOS and TYCHO catalogues. Astrometric and photometric, star catalogues derived from the ESA HIPPARCOS Space Astrometry Mission, ESA SP, 1200
Fischer, D. A., & Valenti, J., 2005, ApJ, 622, 1102
Gaia Collaboration (Prusti, T., et al.) 2016, A&A, 595, A1
Gaia Collaboration (Brown, A. G. A., et al.) 2018, A&A, 616, A1
Garhart, M. P., Smith, M. A., Turnrose, B. E., Levay, K. L., & Thompson, R. W. 1997, IUE NASA Newsletter, 57, 1
Hinz, P. M., Solheid, E., Durney, O., & Hoffmann, W. F. 2008, Proc. SPIE, 7013, 701339
Holland, W. S., Matthews, B. C., Kennedy, G. M., et al. 2017, MNRAS, 470, 3606
Kennedy, G. M., & Kenyon, S. J. 2008, ApJ, 673, 502
Kennedy, G. M., & Kenyon, S. J. 2009, ApJ, 695, 1210
Lafrasse, S., Mella, G., Bonneau, D., et al. 2010, in Optical and Infrared Interferometry II, Proc. SPIE, 7734, 77344E
Lafrenière, D., Marois, C., Doyon, R., Nadeau, D., & Artigau, E. 2007, ApJ, 660, 770
Lagrange, A.-M., Keppler, M., Meunier, N., et al. 2018, A&A, 612, A108
Lannier, J., Lagrange, A. M., Bonavita, M., et al. 2017, A&A, 603, A54
Le Borgne, J.-F., Bruzual, G., Pelló, R., et al. 2003, A&A, 402, 433
Ligi, R., Mourard, D., Lagrange, A. M., et al. 2012, A&A, 545, A5
Ligi, R., Creevey, O., Mourard, D., et al. 2016, A&A, 586, A94
Lindegren, L., Hernández, J., Bombrun, A., et al. 2018, A&A, 616, A2
Mamajek, E. E., & Hillenbrand, L. A. 2008, ApJ, 687, 1264
Marois, C., Lafrenière, D., Doyon, R., Macintosh, B., & Nadeau, D. 2006, ApJ, 641, 556
Meunier, N., Lagrange, A.-M., & De Bondt, K. 2012, A&A, 545, A87
Montesinos, B., Eiroa, C., Krivov, A. V., et al. 2016, A&A, 593, A51
Moór, A., Pascucci, I., Kóspál, A., et al. 2011, ApJS, 193, 4
Mourard, D., Clausse, J. M., Marcotto, A., et al. 2009, A&A, 508, 1073
Mourard, D., Challouf, M., Ligi, R., et al. 2012, Proc. SPIE, 8445, 84450K
Perraut, K., Borgniet, S., Cunha, M., et al. 2013, A&A, 559, A21
Poglitsch, A., Waelkens, C., Geis, N., et al. 2010, A&A, 518, L2
Rhee, J. H., Song, I., Zuckerman, B., & McElwain, M. 2007, ApJ, 660, 1556
Sahlmann, J., Ségransan, D., Queloz, D., et al. 2011, A&A, 525, A95
Skrutskie, M. F., Jones, T., Hinz, P., et al. 2010, Ground-based and Airborne Instrumentation for Astronomy III, Proc. SPIE, 7735, 77353H
Soubiran, C., Le Campion, J.-F., Brouillet, N., & Chemin, L. 2016, A&A, 591, A118
Stassun, K. G., Collins, K. A., & Gaudi, B. S. 2017, AJ, 153, 136
Su, K. Y. L., Morrison, S., Malhotra, R., et al. 2015, ApJ, 799, 146
Su, K. Y. L., De Buizer, J. M., Rieke, G. H., et al. 2017, AJ, 153, 226
Tallon-Bosc, I., Tallon, M., Thiébaut, E., et al. 2008, SPIE Conf. Ser., 7013, 44
ten Brummelaar, T. A., McAlister, H. A., Ridgway, S. T., et al. 2005, ApJ, 628, 453
van Leeuwen, F. 2007, A&A, 474, 653
van Lieshout, R., Dominik, C., Kama, M., & Min, M. 2014, A&A, 571, A51
White, T. R., Huber, D., Mann, A. W., et al. 2018, MNRAS, 477, 4403
Zuckerman, B., & Song, I. 2004, ARA&A, 42, 685
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