Volume 570, October 2014
|Number of page(s)||4|
|Published online||16 October 2014|
The IACOB project⋆
II. On the scatter of O-dwarf spectral type − effective temperature calibrations
Instituto de Astrofísica de Canarias, 38200
La Laguna, Tenerife
2 Departamento de Astrofísica, Universidad de La Laguna, 38205, La Laguna, Tenerife, Spain
3 Departamento de Física, Universidad de La Serena, Av. Cisternas 1200 Norte, La Serena, Chile
4 Centro de Astrobiologìa, CSIC-INTA. Ctra. Torrejón a Ajalvir km. 4, 28850 Torrejón de Ardoz, Madrid, Spain
5 Universitäts-Sternwarte, Scheinerstrasse 1, 81679 München, Germany
6 Argelander Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany
7 UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, UK
Received: 4 August 2014
Accepted: 23 September 2014
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.
Aims. We investigate the spectral type – effective temperature (SpT – Teff) calibration for O-type dwarfs and its claimed dependence on metallicity, using statistically meaningful samples of stars extracted from the IACOB and VFTS surveys.
Methods. We performed a homogeneous differential spectroscopic analysis of 33 Galactic and 53 LMC O dwarfs (spanning spectral types of O4 – O9.7) using the iacob-gbat package, a χ2-fitting algorithm based on a large pre-computed grid of fastwind models, and standard techniques for the hydrogen/helium analysis of O-type stars. We compared the estimated effective temperatures and gravities as a function of (internally consistent) spectral classifications.
Results. While the general trend is that the temperature of a star increases with earlier spectral types and decreasing metallicity, we show that the wide range of gravities found for O-type dwarfs – spaning up to 0.45−0.50 dex in some spectral bins – plays a critical role on the dependence of the effective temperature calibrations as a function of spectral type and metallicity.
Conclusions. This result warns us about the use of SpT - Teff calibrations for O dwarfs that ignore the effects of gravity, and highlights the risks of employing calibrations based on small samples. The effects of this scatter in gravities (evolutionary status) for O-type dwarfs should be included in future recipes that employ SpT - Teff calibrations.
Key words: stars: early-type / stars: fundamental parameters
Based on observations made with (1) the Nordic Optical Telescope, operated on the island of La Palma jointly by Denmark, Finland, Iceland, Norway, and Sweden, in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias, and (2) the European Southern Observatory Very Large Telescope in programme 182.D-0222.
© ESO, 2014
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