First light of the VLT planet finder SPHERE - II. The physical properties and the architecture of the young systems PZ Telescopii and HD 1160 revisited

A.-L. Maire; M. Bonnefoy; C. Ginski; A. Vigan; S. Messina; D. Mesa; R. Galicher; R. Gratton; S. Desidera; T. G. Kopytova; M. Millward; C. Thalmann; R. U. Claudi; D. Ehrenreich; A. Zurlo; G. Chauvin; J. Antichi; A. Baruffolo; A. Bazzon; J.-L. Beuzit; P. Blanchard; A. Boccaletti; J. de Boer; M. Carle; E. Cascone; A. Costille; V. De Caprio; A. Delboulbé; K. Dohlen; C. Dominik; M. Feldt; T. Fusco; J. H. Girard; E. Giro; D. Gisler; L. Gluck; C. Gry; T. Henning; N. Hubin; E. Hugot; M. Jaquet; M. Kasper; A.-M. Lagrange; M. Langlois; D. Le Mignant; M. Llored; F. Madec; P. Martinez; D. Mawet; J. Milli; O. Möller-Nilsson; D. Mouillet; T. Moulin; C. Moutou; A. Origné; A. Pavlov; C. Petit; J. Pragt; P. Puget; J. Ramos; S. Rochat; R. Roelfsema; B. Salasnich; J.-F. Sauvage; H. M. Schmid; M. Turatto; S. Udry; F. Vakili; Z. Wahhaj; L. Weber; F. Wildi

doi:10.1051/0004-6361/201526594

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Volume 587 (March 2016)

A&A, 587 (2016) A56

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Fig. 13

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Comparison of the K1−K2 colors of PZ Tel B and of HD 1160 B and C to those of field dwarfs (yellow squares), young brown dwarfs at the M/L transition (pink circles), and companions to nearby young stars (symbols).

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