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Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2016, Volume 456, Issue 2, pp. 1424 - 1437
Journal Article
Annual review of astronomy and astrophysics, ISSN 1545-4282, 2009, Volume 47, Issue 1, pp. 333 - 370
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 07/2005, Volume 437, Issue 1, pp. 247 - 255
In two papers we try to confirm that all Galactic high-mass stars are formed in a cluster environment, by excluding that O-type stars found in the Galactic field actually formed there. In de Wit et al. (2004... 
Galaxy: stellar content | Stars: kinematics | Stars: early-type | Stars: formation | STELLAR CLUSTERS | ASSOCIATIONS | stars : early-type | MOLECULAR CLOUDS | stars : kinematics | GALAXY | HIPPARCOS | Galaxy : stellar content | EVOLUTION | stars : formation | ASTRONOMY & ASTROPHYSICS | ACCRETION | HERBIG AE/BE STARS | MAGELLANIC CLOUDS | VELOCITIES
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 1365-2966, 2014, Volume 440, Issue 4, pp. 3444 - 3461
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 1365-2966, 2018, Volume 476, Issue 3, pp. 2968 - 2998
.... These dips are too large to be attributed to stellar variability, last from hours to days and can reduce the flux of a star by 10-50 per cent... 
Techniques: photometric | Herbig Ae/Be | Methods: data analysis | Stars: variables: T Tauri | methods: data analysis | techniques: photometric | ASTRONOMY & ASTROPHYSICS | VARIABLE-STARS | CLASSIFICATION | stars: variables: T Tauri, Herbig Ae/Be | SCO | Physics - Solar and Stellar Astrophysics
Journal Article