@article{12162, author = {M. Nowak and S. Lacour and A.-M. Lagrange and P. Rubini and J. Wang and T. Stolker and R. Abuter and A. Amorim and R. Asensio-Torres and M. Bauböck and Jason Dexter and et al.}, title = {Direct confirmation of the radial-velocity planet β Pictoris c}, abstract = {Context. Methods used to detect giant exoplanets can be broadly divided into two categories: indirect and direct. Indirect methods are more sensitive to planets with a small orbital period, whereas direct detection is more sensitive to planets orbiting at a large distance from their host star. This dichotomy makes it difficult to combine the two techniques on a single target at once. Aims. Simultaneous measurements made by direct and indirect techniques offer the possibility of determining the mass and luminosity of planets and a method of testing formation models. Here, we aim to show how long-baseline interferometric observations guided by radial-velocity can be used in such a way. Methods. We observed the recently-discovered giant planet β Pictoris c with GRAVITY, mounted on the Very Large Telescope Interferometer. Results. This study constitutes the first direct confirmation of a planet discovered through radial velocity. We find that the planet has a temperature of T = 1250 ± 50 K and a dynamical mass of M = 8.2 ± 0.8 MJup. At 18.5 ± 2.5 Myr, this puts β Pic c close to a ‘hot start’ track, which is usually associated with formation via disk instability. Conversely, the planet orbits at a distance of 2.7 au, which is too close for disk instability to occur. The low apparent magnitude (MK = 14.3 ± 0.1) favours a core accretion scenario. Conclusions. We suggest that this apparent contradiction is a sign of hot core accretion, for example, due to the mass of the planetary core or the existence of a high-temperature accretion shock during formation.}, year = {2020}, journal = {Astronomy & Astrophysics}, volume = {642}, pages = {L2}, month = {2020-10}, publisher = {EDP Sciences}, issn = {1432-0746}, url = {http://dx.doi.org/10.1051/0004-6361/202039039}, doi = {10.1051/0004-6361/202039039}, }