Heading Gaia to measure atmospheric dynamics in AGB stars
arXiv:1808.02548 · doi:10.1051/0004-6361/201833844
Abstract
Context. Asymptotic Giant Branch stars are characterised by complex stellar surface dynamics that affect the measurements and amplify the uncertainties on stellar parameters. The resulting motion of the stellar photo-center could have adverse effects on the parallax determination with Gaia. Aims. We explore the impact of the convection-related surface structure in AGBs on the photocentric variability. We quantify these effects to characterise the observed parallax errors and estimate fundamental stellar parameters and dynamical properties. Methods. We use 3D radiative-hydrodynamics simulations of convection with CO5BOLD and the post-processing radiative transfer code Optim3D to compute intensity maps in the Gaia G band. From those maps, we calculate the intensity-weighted mean of all emitting points tiling the visible stellar surface and evaluate its motion as a function of time. We extract the parallax error from Gaia DR2 for a sample of semiregular variables in the solar neighbourhood and compare it to the synthetic predictions of photo-center displacements. Results. AGB stars show a complex surface morphology characterised by the presence of few large scale long-lived convective cells accompanied by short-lived and small scale structures. As a consequence, the position of the photo-center displays temporal excursions between 0.077 to 0.198 AU (5 to 11% of the corresponding stellar radius), depending on the simulation considered. We show that the convection-related variability accounts for a substantial part to the Gaia DR2 parallax error of our sample of semiregular variables. Finally, we put in evidence for a correlation between the mean photo-center displacement and the stellar fundamental parameters: surface gravity, radius, and pulsation. We denote that parallax variations could be exploited quantitatively using appropriate RHD simulations corresponding to the observed star.
arXiv commentLetter to the Editor. Accepted for publication on Astronomy & Astrophysics
References in corpus (17)
- The chemical composition of the Sun
- Gaia Data Release 2. Summary of the contents and survey properties
- The Gaia mission
- A grid of MARCS model atmospheres for late-type stars I. Methods and general properties
- Estimating distances from parallaxes IV: Distances to 1.33 billion stars in Gaia Data Release 2
- Gaia Data Release 2: Photometric content and validation
- Gaia Data Release 2: Catalogue validation
- On the use of empirical bolometric corrections for stars
- Simulations of stellar convection with CO5BOLD
- Gaia Data Release 1: Catalogue validation
- Radiative hydrodynamics simulations of red supergiant stars: I. interpretation of interferometric observations
- Global 3D radiation-hydrodynamics models of AGB stars. Effects of convection and radial pulsations on atmospheric structures
- Radiative hydrodynamics simulations of red supergiant stars. III. Spectro-photocentric variability, photometric variability, and consequences on Gaia measurements
- AGB Stars in the Fornax Dwarf Spheroidal Galaxy
- Hydrodynamical simulations of convection-related stellar micro-variability. I. Statistical relations for photometric and photocentric variability
- Long-term photometry and periods for 261 nearby pulsating M giants
- Semi-Regular Variables in the Solar Neighbourhood
Cited by in corpus (30)
- Stellar and substellar companions of nearby stars from Gaia DR2 - Binarity from proper motion anomaly
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- Distance estimates for AGB stars from parallax measurements
- Numerical Simulations of Convective 3-Dimensional Red Supergiant Envelopes
- Microarcsecond Astrometry: Science Highlights from Gaia
- The period-luminosity relation of red supergiants with Gaia DR2
- Exploring the origin of clumpy dust clouds around cool giants. A global 3D RHD model of a dust-forming M-type AGB star
- Global 3D radiation-hydrodynamical models of AGB stars with dust-driven winds
- The Mira Distance to M101 and a 4% Measurement of H0
- Properties of carbon stars in the Solar neighbourhood based on Gaia DR2 astrometry
- The period--luminosity relation for Mira variables in the Milky Way using Gaia DR3: a further distance anchor for
- A Dramatic Decrease in Carbon Star Formation in M31
- A Fresh Look at AGB stars in Galactic Open Clusters with Gaia: Impact on Stellar Models and the Initial-Final Mass Relation
- Multiwavelength Period-Luminosity and Period-Luminosity-Color relations at maximum-light for Mira variables in the Magellanic Clouds
- The abundance of S- and Si-bearing molecules in O-rich circumstellar envelopes of AGB stars
- Probing Red Supergiant dynamics through photo-center displacements measured by Gaia
- High-resolution spectroscopic study of massive blue and red supergiants in Per OB1
- A kinematic calibration of the O-rich Mira variable period-age relation from Gaia
- Optical interferometry and Gaia measurement uncertainties reveal the physics of asymptotic giant branch stars
- A Census of Thermally-Pulsing AGB stars in the Andromeda Galaxy and a First Estimate of their Contribution to the Global Dust Budget
- The extended atmosphere and circumstellar environment of the cool evolved star VX Sagittarii as seen by MATISSE
- Annual parallax measurement of a Mira variable star BX Cam with VERA
- Tomography of cool giant and supergiant star atmospheres III. Validation of the method on VLTI/AMBER observations of the Mira star S Ori
- Long-Period High-Amplitude Red Variables in the KELT Survey
- A Non-Detection of Red Supergiant Convection in Gaia
- Characterizing the Evolved Stellar Population in the Galactic Foreground I: Bolometric Magnitudes, Spatial Distribution and P-L Relations
- The frequency by mass of Galactic carbon stars inferred from Gaia measurements of star cluster members
- Extended view on the dust shells around two carbon stars
- Water vapour masers in long-period variable stars III. Mira variables U Her and RR Aql
- The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope