2014/09/23 by S. Simón-Díaz, A. Herrero, C. Sabín-Sanjulián +6 · 1 citation
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Calibration #Effective temperature #Function (biology) #Gamma-ray bursts and supernovae #Geology #Homogeneous #Metallicity #Physics #Spectral line #Stars #Statistical physics #Stellar classification #Stellar, planetary, and galactic studies #Surface gravity #Type (biology) #astro-ph.SR
paper · pdf · doi:10.1051/0004-6361/201424742
published as A&A 570, L6 (2014) · 4 pages, 3 figures, 1 table; accepted fro publication in A&A Letters
arxiv created 2014/09/23 · openalex publication_date 2014/09/25 · arxiv updated 2014/10/22 · openalex created_date 2022/10/04 · openalex updated_date 2026/08/05
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.