The IACOB project⋆

Author： Simón-Díaz S.   Herrero A.   Sabín-Sanjulián C.   Najarro F.   Garcia M.   Puls J.   Castro N.   Evans C. J.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|570|issue|L6-L6

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.570, Iss.issue, 2014-10, pp. : L6-L6

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

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Abstract

Context. We are now in an era of large spectroscopic surveys of OB-type stars. Quantitative spectroscopic analysis of these modern datasets is enabling us to review the physical properties of blue massive stars with robust samples, not only revisiting mean properties and general trends, but also incorporating information about the effects of second-order parameters.

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