Modelling the asymmetric wind of the luminous blue variable binary MWC 314

Abstract

We present a spectroscopic analysis of MWC 314, a luminous blue variable (LBV) candidate with an extended bipolar nebula. The detailed spectroscopic variability is investigated to determine if MWC 314 is a massive binary system with a supersonically accelerating wind or a low-mass B[e] star. We compare the spectrum and spectral energy distribution to other LBVs (such as P Cyg) and find very similar physical wind properties, indicating strong kinship. We combined long-term high-resolution optical spectroscopic monitoring and V-band photometric observations to determine the orbital elements and stellar parameters and to investigate the spectral variability with the orbital phases. We developed an advanced model of the large-scale wind-velocity and wind-density structure with 3-D radiative transfer calculations that fit the orbitally modulated P Cyg profile of He I lam5876, showing outflow velocities above 1000 km/s. We find that MWC 314 is a massive semi-detached binary system of ~1.22 AU, observed at an inclination angle of i=72.8 deg. with an orbital period of 60.8 d and e=0.23. The primary star is a low-vsini LBV candidate of m1=39.6 Msun and R1=86.8 Rsun. The detailed radiative transfer fits show that the geometry of wind density is asymmetric around the primary star with increased wind density by a factor of 3.3, which leads the orbit of the primary. The variable orientation causes the orbital modulation that is observed in absorption portions of P Cyg wind lines. Wind accretion in the system produces a circumbinary disc. MWC 314 is in a crucial evolutionary phase of close binary systems, when the massive primary star has its H envelope being stripped and is losing mass to a circumbinary disc. MWC 314 is a key system for studying the evolutionary consequences of these effects.

14 pages, 25 figures, 4 tables, Accepted for Astronomy and Astrophysics

References in corpus (8)

• The SCUBA Legacy Catalogue: Continuum Objects Detected by SCUBA
• Chemical evolution of galaxies. I. A composition-dependent SPH model for chemical evolution and cooling
• Calibrated griz magnitudes of Tycho stars: All-sky photometric calibration using bright stars
• Modeling Ultraviolet Wind Line Variability in Massive Hot Stars
• A multispectral view of the periodic events in eta Carinae
• Possible Implications of Mass Accretion in Eta Carinae
• Spectral atlas of massive stars around He I 10830 A
• The Asymmetrical Wind of the Candidate Luminous Blue Variable MWC 314

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