1. Correlating Changes in Spot Filling Factors with Stellar Rotation
- Author
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Perez Paolino, F, Bary, J, Petersen, M, Ward-Duong, K, Follete, K, Brun, Allan Sacha, Bouvier, Jérôme, and Petit, Pascal
- Subjects
Starspots, Pre-main Sequence Stars, T-Tauri Stars, Early Stellar Evolution, Star Formation - Abstract
Using a multi-epoch near-infrared spectroscopic dataset of three heavily-spotted T Tauri star systems we use empirical composite spectral models to constrain spot filling factors and temperatures. Empirical composite models are created through a weighted sum of two IRTF Spectral Library dwarf standard spectra, a cooler one for the spots and a hotter one for the photosphere, and then fit to each observed stellar spectra using a Markov-Chain Monte-Carlo algorithm. Fits to individual epochs reveal clear variations in filling factors that are correlated with photometric variability. Covering over one full stellar enables us to calculate the total spot coverage of the stars. Knowing this, we revise the HR diagram placement of our sample and obtain new mass and age estimates using traditional unspotted and new spotted evolutionary models. Our results suggest that a failure to account for spots results in mass and age spreads as large as a factor of two. Additionally, analysis of AAVSO photometric data reveals evidence for spot evolution on timescales as short as a few years., {"references":["Strassmeier, K. G., \"Starspots\", A&A Rev, 2009. doi:10.1007/s00159-009-0020-6","Gully-Santiago, M. A., \"Placing the Spotted T Tauri Star LkCa 4 on an HR Diagram\", ApJ, 2017. doi:10.3847/1538-4357/836/2/200","Luger, R., Foreman-Mackey, D., and Hedges, C., \"starry_process: Interpretable Gaussian processes for stellar light curves\", JOSS, 2021. doi:10.21105/joss.03071","Roettenbacher, R. M., \"Contemporaneous Imaging Comparisons of the Spotted Giant σ Geminorum Using Interferometric, Spectroscopic, and Photometric Data\", ApJ, 2017. doi:10.3847/1538-4357/aa8ef7","Somers, G., Cao, L., and Pinsonneault, M. H., \"The SPOTS Models: A Grid of Theoretical Stellar Evolution Tracks and Isochrones for Testing the Effects of Starspots on Structure and Colors\", ApJ, 2020","Baraffe, I., Homeier, D., Allard, F., and Chabrier, G., \"New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit\", A&A, 2015. doi:10.1051/0004-6361/201425481. doi:10.3847/1538-4357/ab722e"]}
- Published
- 2022
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