PhD thesis developed in the framework of the IACOB project
- A. Casasbuenas (started 2023), "Improving the reliability of surface abundance determinations in OB stars"
- C. Martínez Sebastíán (started 2022), "A massive empirical approach to stellar evolution with IACOB, WEAVE and Gaia"
- A. de Burgos (started 2019), "On the evolutionary nature of massive B-type supergiants: a modern empirical reappraisal using data from IACOB, Gaia and TESS"
- G. Holgado (2019), "Spectroscopic and physical characterization of the Galactic O-type stars surveyed by the IACOB and OWN surveys"
Some other PhD thesis of interest
From the IAC group:
- S. R. Berlanas (2019), "Massive stars in Cygnus OB2"
- K. Rübke (2017), " Massive obscured clusters in the Milky Way "
- I. Camacho (2017), " The impact of metallicity on massive star evolution "
- C. Sabín-Sanjulian (2014), "Quantitative spectroscopic analysis of O-type stars in the 30 Doradus region of the LMC"
- S. Ramirez-Alegria (2012), "Cúmulos Estelares Masivos Oscurecidos en la Vía Láctea"
- N. Castro (2010), " An study of extragalactic massive stars "
- S. Simón-Díaz (2005), " Interaction between massive stars and the interstellar medium in Galactic HII regions "
- M. Garcia (2005), "A study of Massive Stars from high resolution spectroscopy in the F-UV, UV and optical ranges"
- M. A. Urbaneja (2004), " B Supergiants in the Milky way and nearby galaxies: models and quantitative spectroscopy "
- M. R. Villamariz (2000), "Spectroscopic analysis of Galactic OB stars"
- E. Santolaya-Rey (1995), "Unified Models for the Analysis of Hot Star Atmospheres"
From the KULeuven groups:
- S. Burssens (2022): " Massive star asteroseismology with K2 and TESS "
- C. Hawcroft (2022): " Stellar wind properties of O-type stars: mass loss, speeds, structure and quantitative empirical analysis "
- R. Björklund (2021): " Radiation-driven mass loss and its effect on massive-star evolution "
- J. Bodensteiner (2021): " Observational imprints of binary evolution on B- and Be-star populations "
- M. Abdul-Masih (2020): " Spectroscopy of spherically distorted massive stars: testing internal mixing and stellar evolution "
- C. Johnston (2020): " Interior modelling of massive stars in multiple systems "
- M. G. Pedersen (2020): " Interior rotation, mixing and ages of a sample of Slowly Pulsating B stars from gravity-mode asteroseismology "
- G. Raskin (2011): " Hermes, a fibre-fed high-resolution spectrograph for the Mercator Telescope "
- P. Degroote (2010): " Asteroseismology of OB stars with the Corot Space mission "
- B. Buysschaert (2018): " Asteroseismology of magnetic massive stars "
- K. Lefever (2007): " Fundamental parameters of B-type stars. Application to a HIPPARCOS sample of B supergiants and a CoRoT sample of B dwarfs "
From the Bonn group:
- C. Wang (2022): " The impact of binary interaction on the main-sequence morphology of young star clusters "
- A. Schootemeijer (2018): " The evolution of massive stars in the Small Magellanic Cloud "
- P. Marchant (2017): " The impact of tides and mass transfer on the evolution of metal-poor massive binary stars "
- L. Grassitelli (2016), "Instabilities in the envelopes of stars"
- K. Köhler (2016): " Massive stars on the main sequence "
- D. Sanyal (2016): " Envelope inflation in massive stars near the Eddington limit "
- D. Szécsi (2016): " The evolution of low-metallicity massive stars "
- F. Schneider (2014), "Statistical analyses of massive stars and stellar popullations"
- I. Brott (2011), "Modelling populations of rotationally mixed massive stars"
- L. Muijres (2010): " The physics of line-driven winds of hot massive stars "
- S. E. de Mink (2009), "Stellar evolution at low metallicity under the influence of binary interaction and rotation"
- M. Cantiello (2009), "Observational consequences of instable stellar interiors"
- J. Petrovic (2004): " On the Evolution of Massive Close Binary Systems "
- A. Heger (1998): "The Pre-Supernova Evolution of Rotating Massive Stars"
From the CAB group:
- M. M. Rubio Díez (2020), "A multi-wavelegth view of stellar evolution in massive stars: re-examining the upper mass limit and constraining the mass-loss rate"
From the Amsterdam group:
- Zapartas, E. (2018): "The deaths of massive stars in binary systems"
- Lenorzer, A. (2004): "Near-infrared spectroscopic analysis of hot massive stars"
- Mokiem, M. R. (2006): "The physical properties of early-type massive stars"
- Ramírez Tannus, M. C. (2018): "The outcome of massive star formation"
- Muijres, L. E. (2010): "The physics of line-driven winds of hot massive stars"
- Tramper, F. (2014): "The properties of low-metallicity massive stars"
- Ramírez Agudelo, O. H. (2015): Properties of massive stars in the Tarantula Nebula"
From the Genève group:
- S. Ekstron (2008): "The evolution of fast rotating massive stars at low or zero metallicity"
- R. Hisrschi (2004): "Massive rotating stars : the road to supernova explosion"
From the Queen's University group:
- Z. Keszthelyi (2019): " The role of surface fossil magnetic fields in massive star evolution "
- A. David-Uraz (2016): " Investigating the potential magnetic origin of wind variability in OB stars "
- M. Shultz (2016): " The Rotational Evolution and Magnetospheric Emission of the Magnetic Early B-type Stars "
- J. Grunhut (2012): " A detailed observational analysis of magnetism in three B and O stars observed within the context of the MiMeS project "
Other PhD thesis:
- A. Irrgang (2014), "Origin of runaway OB stars"
- L. Mahy (2011), "Astrophysical parameters and multiplicity of massive stars: a mathematical approach"
- T. Repolust (2005), "Quantitative spectroscopy of OB-stars in the optical and the Infrared"
- F. Martins (2004), "New atmosphere models for massive stars: line-blanketing effects and win properties of O-type stars"
- N. Przybilla (2002), "Quantitative spectroscopy of supergiants"
- F. Najarro (1995), "Quantitative optical and infrared spectroscopy of extreme Luminous Blue Supergiants
- A. Herrero (1986), "NLTE Line Formation Calculations for Hydrogen and Ionized Helium in Photospheres of Very Hot Stars"