DOI,IST REx ID,Title of publication
10.1051/0004-6361/201935684,13470,"The Wolf–Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud"
10.1051/0004-6361/201833297,13471,Massive runaway and walkaway stars
10.1051/0004-6361/201732206,13472,No surviving non-compact stellar companion to Cassiopeia A
10.1051/0004-6361/201834916,6756,Unexpected topology of the temperature fluctuations in the cosmic microwave background
10.1051/0004-6361/201833528,11508,Confirmation of double peaked Lyα emission at z = 6.593: Witnessing a galaxy directly contributing to the reionisation of the universe
10.1051/0004-6361/201833106,11618,FliPer: A global measure of power density to estimate surface gravities of main-sequence solar-like stars and red giants
10.1051/0004-6361/201834289,11619,"TESS’s first planet: A super-Earth transiting the naked-eye star π Mensae"
10.1051/0004-6361/201731194,13473,"Clues about the scarcity of stripped-envelope stars from the evolutionary state of the sdO+Be binary system φ Persei"
10.1051/0004-6361/201732274,13475,Spectral models for binary products: Unifying subdwarfs and Wolf-Rayet stars as a sequence of stripped-envelope stars
10.1051/0004-6361/201730472,13476,Ionizing spectra of stars that lose their envelope through interaction with a binary companion: Role of metallicity
10.1051/0004-6361/201629685,13477,Delay-time distribution of core-collapse supernovae with late events resulting from binary interaction
10.1051/0004-6361/201526309,13478,Long-term stability of the HR 8799 planetary system without resonant lock