HR 6819 is a binary system with no black hole Revisiting the source with infrared interferometry and optical integral field spectroscopy

Frost, AJ; Bodensteiner, J; Rivinius, Th; Baade, D; Merand, A; Selman, F; Abdul-Masih, M; Banyard, G; Bordier, E; Dsilva, K; Hawcroft, C; Mahy, L; Reggiani, M; Shenar, T; Cabezas, M; Hadrava, P; Heida, M; Klement, R; Sana, H

doi:10.1051/0004-6361/202143004

HR 6819 is a binary system with no black hole Revisiting the source with infrared interferometry and optical integral field spectroscopy

Author:

Frost, AJ

Bodensteiner, J ; Rivinius, Th ; Baade, D ; Merand, A ; Selman, F ; Abdul-Masih, M ; Banyard, G ; Bordier, E ; Dsilva, K ; Hawcroft, C ; Mahy, L ; Reggiani, M ; Shenar, T ; Cabezas, M ; Hadrava, P ; Heida, M ; Klement, R ; Sana, H

Keywords:

Science & Technology, Physical Sciences, Astronomy & Astrophysics, stars: individual: HR 6819, stars: massive, stars: emission-line, Be, binaries: close, techniques: interferometric, techniques: imaging spectroscopy, STARS, MULTIPLES - 772225;info:eu-repo/grantAgreement/EC/H2020/772225, 0201 Astronomical and Space Sciences, 5101 Astronomical sciences, 5107 Particle and high energy physics, 5109 Space sciences