_id,doi,title
13466,10.1051/0004-6361/201936743,The young massive SMC cluster NGC 330 seen by MUSE
13467,10.1051/0004-6361/201936669,Contribution from stars stripped in binaries to cosmic reionization of hydrogen and helium
11499,10.1051/0004-6361/201834565,"Exploring He II λ1640 emission line properties at z ∼2−4"
11505,10.1051/0004-6361/201834471,"Faint end of the z ∼ 3–7 luminosity function of Lyman-alpha emitters behind lensing clusters observed with MUSE"
11507,10.1051/0004-6361/201833075,Predicting Lyα escape fractions with a simple observable: Lyα in emission as an empirically calibrated star formation rate indicator
11614,10.1051/0004-6361/201834780,FliPerClass: In search of solar-like pulsators among TESS targets
13468,10.1051/0004-6361/201935854,The diverse lives of progenitors of hydrogen-rich core-collapse supernovae: The role of binary interaction
13469,10.1051/0004-6361/201834525,The impact of stars stripped in binaries on the integrated spectra of stellar populations
13470,10.1051/0004-6361/201935684,"The Wolf–Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud"
13471,10.1051/0004-6361/201833297,Massive runaway and walkaway stars
13472,10.1051/0004-6361/201732206,No surviving non-compact stellar companion to Cassiopeia A
11508,10.1051/0004-6361/201833528,Confirmation of double peaked Lyα emission at z = 6.593: Witnessing a galaxy directly contributing to the reionisation of the universe
11618,10.1051/0004-6361/201833106,FliPer: A global measure of power density to estimate surface gravities of main-sequence solar-like stars and red giants
11619,10.1051/0004-6361/201834289,"TESS’s first planet: A super-Earth transiting the naked-eye star π Mensae"
13473,10.1051/0004-6361/201731194,"Clues about the scarcity of stripped-envelope stars from the evolutionary state of the sdO+Be binary system φ Persei"
13475,10.1051/0004-6361/201732274,Spectral models for binary products: Unifying subdwarfs and Wolf-Rayet stars as a sequence of stripped-envelope stars
13476,10.1051/0004-6361/201730472,Ionizing spectra of stars that lose their envelope through interaction with a binary companion: Role of metallicity
13477,10.1051/0004-6361/201629685,Delay-time distribution of core-collapse supernovae with late events resulting from binary interaction
13478,10.1051/0004-6361/201526309,Long-term stability of the HR 8799 planetary system without resonant lock