Fundamental properties of two rapidly rotating stars: Rasalhague and Alkaid

Abstract

Abridged : The fundamental parameters of rapidly rotating stars are key quantities to understand the impact of rotation on stellar evolution. A few nearby early-type stars offer the possibility of precise measurements of these parameters, which will help us constrain newly available two-dimensional models. We propose a method to retrieve the fundamental parameters of a fast rotating star (mass, rotation rate, and age), and also the inclination of its rotation axis on the line of sight, using five spectrophotometric observables along with a set of steady 2D-models. Using the temperature derived by the infrared flux method, the Vsini and the apparent luminosity, along with a grid of 2D steady state models, we select models that are compatible with all observational constraints, and derive the most probable mass, rotation rate, core hydrogen mass fraction relative to that of the envelope, and inclination of the rotation axis on the line of sight of the targetted star. We apply this method to two stars: Rasalhague (alpha Oph) and Alkaid (eta UMa). We confirm and improve the fundamental parameters of Rasalhague and provide a new determination of its rotation axis inclination on the line-of-sight, which we find to be $\sim 69$ degrees. Concerning Alkaid, we infer a mass of $5.071\pm 0.023M_{\odot }$, a rotation rate corresponding to an equatorial rotation period of 14.6 hours. We also find an inclination of the rotation axis of $\sim 42$ degrees. We show that Alkaid is a very young star, presumably between 2 and 8 Myrs off the Zero-Age Main Sequence. As a side result, using high resolution spectra and the Least Square Deconvolution method, we determined a precise value of the Vsini of Rasalhague, namely $224.3\pm 2.6$ km/s. Similarly, we find $V\sin i=154.3\pm 9.1$ km/s for Alkaid.

arXiv comment9 pages, 8 figures, accepted for publication in Astronomy & Astrophysics

References in corpus (30)

• The chemical composition of the Sun
• Modules for Experiments in Stellar Astrophysics (MESA)
• Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars
• Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions
• Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions
• The VizieR database of Astronomical Catalogues
• The NextGen Model Atmosphere grid for $3000\le \Teff \le 10000\K$
• Modules for Experiments in Stellar Astrophysics (MESA): Time-Dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure
• Gravity darkening in rotating stars
• Rotational velocities of A-type stars IV. Evolution of rotational velocities
• Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer
• PolarBase: a data base of high resolution spectropolarimetric stellar observations
• A new catalogue of Stroemgren-Crawford uvbybeta photometry
• Resolving Vega and the inclination controversy with CHARA/MIRC
• Self-consistent 2D models of fast rotating early-type star
• Imaging and Modeling Rapidly Rotating Stars: Alpha Cephei and Alpha Ophiuchi
• Automated spectroscopic abundances of A and F-type stars using echelle spectrographs II. Abundances of 140 A-F stars from ELODIE and CORALIE
• An algorithm for computing the 2D structure of fast rotating stars
• Rotationally-modulated g-modes in the rapidly-rotating delta Scuti star Rasalhague (alpha Ophiuchi)
• Polarization due to rotational distortion in the bright star Regulus
• A realistic two-dimensional model of Altair
• The IACOB project XII. A new grid of northern standards for the spectral classification of B-type stars
• Predictions for gravity-mode periods and surface abundances in intermediate-mass dwarfs from shear mixing and radiative levitation
• The first two-dimensional stellar structure and evolution models of rotating stars
• Performance and first measurements of the MAGIC Stellar Intensity Interferometer
• The rotation of alpha Oph investigated using polarimetry
• A Correction for IUE UV Flux Distributions from Comparisons with CALSPEC
• Vintage NPOI: New and Updated Angular Diameters for 145 Stars
• Photometric determination of rotation axis inclination, rotation rate, and mass of rapidly rotating intermediate-mass stars
• Halo Photometry and Asteroseismology for 98 of the Brightest Stars Observed by TESS