中文
相关论文

相关论文: Spectral characterization and differential rotatio…

200 篇论文

About 10% of upper main sequence stars are characterised by the presence of chemical peculiarities, often found together with a structured magnetic field. The atmospheres of most of those chemically peculiar stars present surface spots,…

太阳与恒星天体物理 · 物理学 2015-06-03 K. T. Wraight , L. Fossati , M. Netopil , E. Paunzen , M. Rode-Paunzen , D. Bewsher , A. J. Norton , G. J. White

Analyses of very accurate CoRoT space photometry, past Johnson V photoelectric photometry and high-resolution \'echelle spectra led to the determination of improved and consistent fundamental stellar properties of both components of AU Mon.…

We provide CoRoT and Spitzer light curves, as well as broad-band multi-wavelength photometry and high resolution, multi- and single-epoch spectroscopy for 17 classical T Tauris in NGC 2264 whose CoRoT light curves (LCs) exemplify the…

With the advent of space-based precision photometry missions the quantity and quality of starspot light curves has greatly increased. This paper presents a large number of starspot models and their resulting light curves to: 1) better…

太阳与恒星天体物理 · 物理学 2020-08-13 Gibor Basri , Riya Shah

Starspots are cooler and darker than the stellar surface. Therefore, the emitted flux of a star changes when spots are visible on its surface. The presence of spots together with the stellar rotation leads to a periodic modulation on the…

太阳与恒星天体物理 · 物理学 2017-11-08 A. R. G. Santos , M. S. Cunha , P. P. Avelino , R. A. García , S. Mathur

Our goal is to determine the rotational and magnetic-related activity properties of stars at different stages of evolution. We have focussed our attention on 6 young loose stellar associations within 100 pc and ages in the range 8-70 Myr:…

太阳与恒星天体物理 · 物理学 2017-03-15 S. Messina , S. Desidera , M. Turatto , A. C. Lanzafame , E. F. Guinan

I briefly review the current state of the modelling of photospheric activity based on the high-precision optical light curves obtained with MOST, CoRoT, and Kepler. These models can be used to search for active longitudes where activity is…

太阳与恒星天体物理 · 物理学 2015-06-04 A. F. Lanza

We report the discovery of a new relationship between a simple morphological characteristic of light curves produced by starspots and stellar rotation periods. The characteristic we examine is whether the light curve exhibits one dip or two…

太阳与恒星天体物理 · 物理学 2018-08-29 Gibor Basri , Hieu T. Nguyen

We investigate the photometric modulation induced by magnetic activity cycles and study the relationship between rotation period and activity cycle(s) in late-type (FGKM) stars. We analyse light-curves spanning up to 9 years of 125 nearby…

太阳与恒星天体物理 · 物理学 2016-10-26 A. Suárez Mascareño , R. Rebolo , J. I. González Hernández

We present an analytic model of the lightcurve variation for stars with non-evolving starspots on a differentially rotating surface. The Fourier coefficients of the harmonics of the rotation period are expressed in terms of the latitude of…

太阳与恒星天体物理 · 物理学 2022-08-17 Yasushi Suto , Shin Sasaki , Yuta Nakagawa , Othman Benomar

We present the results of numerical experiments to assess degeneracies in lightcurve models of starspots. Using synthetic lightcurves generated with the Cheetah starspot modeling code, we explore the extent to which photometric light curves…

天体物理仪器与方法 · 物理学 2015-06-12 Lucianne M. Walkowicz , Gibor S. Basri , Jeff A. Valenti

Context. The CoRoT short runs give us the opportunity to observe a large variety of late-type stars through their solar-like oscillations. We report observations of the star HD175726 that lasted for 27 days during the first short run of the…

For 6 years the Convection, Rotation, and Planetary Transits (CoRoT) space mission has acquired photometric data from more than one hundred thousand point sources towards and directly opposite from the inner and outer regions of the Galaxy.…

CoRoT 223992193 is the only known low-mass, pre-main sequence eclipsing binary that shows evidence of a circumbinary disk. The system displays complex photometric and spectroscopic variability over a range of timescales and wavelengths.…

Using the wealth of ~24 yr multiband data, we present an in-depth study of the star-spot cycles, surface differential rotations (SDR), optical flares, evolution of star-spot distributions, and coronal activities on the surface of young,…

太阳与恒星天体物理 · 物理学 2016-08-24 Subhajeet Karmakar , J. C. Pandey , I. S. Savanov , G. Taş , S. B. Pandey , K. Misra , S. Joshi , E. S. Dmitrienko , T. Sakamoto , N. Gehrels , T. Okajima

With now more than 20 exoplanets discovered by CoRoT, it has often been considered strange that so many of them are orbiting F-stars, and so few of them K or M-stars. Although transit search programs are mostly sensitive to short-period…

地球与行星天体物理 · 物理学 2015-06-05 E. W. Guenther , D. Gandolfi , D. Sebastian , M. Deleuil , C. Moutou , F. Cusano

We present an analysis of the starspot evolution, the surface differential rotation (SDR), the correlation between chromospheric activity indicators and the spatial connection between chromospheric and photospheric activities on the active…

太阳与恒星天体物理 · 物理学 2021-01-11 Fukun Xu , Shenghong Gu , Panogiotis Ioannidis

The space experiment CoRoT will provide continuous monitoring and high accuracy light curves of about sixty thousand stars. Selected binary systems will be observed in the Additional Program frame as targets of long and continuous pointed…

天体物理学 · 物理学 2016-08-30 Carla Maceroni , Ignasi Ribas

According to earlier Doppler images of the magnetically active primary giant component of the RS CVn binary II Peg, the surface of the star was dominated by one single active longitude that was clearly drifting in the rotational frame of…

The SRa02 of the CoRoT space mission for Asteroseismology was partly devoted to stars belonging to the Mon OB2 association. An intense monitoring was performed on Plaskett's Star (HD47129) and the unprecedented quality of the light curve…

太阳与恒星天体物理 · 物理学 2015-05-20 L. Mahy , E. Gosset , F. Baudin , G. Rauw , M. Godart , T. Morel , P. Degroote , C. Aerts , R. Blomme , J. Cuypers , A. Noels , E. Michel , A. Baglin , M. Auvergne , C. Catala , R. Samadi