The IACOB project: A new Era in the Study of Galactic OB Stars

Start year
2014
End year
2017
Organizational Unit

Grants related:

    General
    Description

    IACOB is an ambitious long-term project whose main scientific goal is to provide an unprecedented empirical overview of the main physical properties of Galactic massive O- and B-type stars which can be used as definitive anchor point for our theories of stellar atmospheres, winds, interiors and evolution of massive stars

    Principal investigator
    Collaborators
    Dr.
    KLAUS SIMON RUBKE ZUÑIGA
    Dr.
    INÉS CAMACHO IÑESTA
    Dr.
    Jesús Maíz Apellaniz
    Dr.
    Ignacio Negueruela
    Dr.
    Norberto Castro
    Dr.
    Carolina Sabín-Sanjulian
    Dr.
    Javier Lorenzo
    Dr.
    Ricardo Dorda e
    Dr.
    María Fernanda Nieva
    Dr.
    Jorge García-Rojas
    Dr.
    Nevy Markova
    Dr.
    Miguel A. Urbaneja

    Related publications

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    • The Cocoon nebula and its ionizing star: do stellar and nebular abundances agree?

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    • Spectroscopic and physical parameters of Galactic O-type stars. II. Observational constraints on projected rotational and extra broadening velocities as a function of fundamental parameters and stellar evolution

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