Photometric and spectroscopic studies of massive binaries in the large MAGELLANIC CLOUD. I. Introduction and orbits for two detached systems: Evidence for a mass discrepancy?

Philip Massey, Nidia I. Morrell, Kathryn F. Neugent, Laura R. Penny, Kathleen D Eastwood, Douglas R. Gies

Research output: Contribution to journalArticle

32 Citations (Scopus)

Abstract

The stellar mass-luminosity relation is poorly constrained by observations for high-mass stars. We describe our program to find eclipsing massive binaries in the Magellanic Clouds using photometry of regions rich in massive stars, and our spectroscopic follow-up to obtain radial velocities and orbits. Our photometric campaign identified 48 early-type periodic variables, of which only 15 (31%) were found as part of the microlensing surveys. Spectroscopy is now complete for 17 of these systems, and in this paper we present analysis of the first two, LMC 172231 and ST2-28, simple detached systems of late-type O dwarfs of relatively modest masses. Our orbit analysis yields very precise masses (2%), and we use tomography to separate the components and determine effective temperatures by model fitting, necessary for determining accurate (0.05-0.07 dex) bolometric luminosities in combination with the light-curve analysis. Our approach allows more precise comparisons with evolutionary theory than previously possible. To our considerable surprise, we find a small, but significant, systematic discrepancy: all of the stars are slightly undermassive, by typically 11% (or overluminous by 0.2 dex) compared with that predicted by the evolutionary models. We examine our approach for systematic problems, but find no satisfactory explanation. The discrepancy is in the same sense as the long-discussed and elusive discrepancy between the masses measured from stellar atmosphere analysis with the stellar evolutionary models, and might suggest that either increased rotation or convective overshooting is needed in the models. Additional systems will be discussed in future papers of this series, and will hopefully confirm or refute this trend.

Original languageEnglish (US)
Article number96
JournalAstrophysical Journal
Volume748
Issue number2
DOIs
StatePublished - Apr 1 2012

Fingerprint

orbits
luminosity
stars
stellar atmospheres
stellar models
Magellanic clouds
stellar mass
massive stars
evolutionary theory
radial velocity
light curve
photometry
tomography
trends
spectroscopy
analysis
atmosphere
temperature

Keywords

  • binaries: eclipsing
  • binaries: spectroscopic
  • stars: early-type
  • stars: fundamental parameters

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Photometric and spectroscopic studies of massive binaries in the large MAGELLANIC CLOUD. I. Introduction and orbits for two detached systems : Evidence for a mass discrepancy? / Massey, Philip; Morrell, Nidia I.; Neugent, Kathryn F.; Penny, Laura R.; Eastwood, Kathleen D; Gies, Douglas R.

In: Astrophysical Journal, Vol. 748, No. 2, 96, 01.04.2012.

Research output: Contribution to journalArticle

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