Results 21 to 30 of about 4,942 (197)

On the parameter refinement of inflated exoplanets with large radius uncertainty based on TESS observations

open access: yesAstronomische Nachrichten, Volume 343, Issue 3, March 2022., 2022
Abstract We revisited 10 known exoplanetary systems using publicly available data provided by the transiting exoplanet survey satellite (TESS). The sample presented in this work consists of short period transiting exoplanets, with inflated radii and large reported uncertainty on their planetary radii.
Xanthippi Alexoudi
wiley   +1 more source

The effect of starspots on the radii of low-mass pre-main sequence stars [PDF]

open access: yes, 2014
A polytropic model is used to investigate the effects of dark photospheric spots on the evolution and radii of magnetically active, low-mass ...
Jackson, R. J., Jeffries, R. D.
core   +10 more sources

Monitoring active stars 29 Dra, 12 Cam and colour excess of II Peg [PDF]

open access: yesSerbian Astronomical Journal, 2007
We present the BV light curves analysis of late-type, long-period stars 29 Dra, 12 Cam for the season 2005/2006, and shorter-period star II Peg for the same season.
Zboril M.
doaj   +1 more source

Starspot Activity without Pulsation in the Binary System KIC 5444392 Revisited

open access: yesUniverse, 2023
We revisited the short-period (∼1.5 days) binary system KIC 5444392, which shows quasi-period modulated light variations. Previous studies indicated that these variations might be caused by stellar pulsations.
Mengqi Jin   +3 more
doaj   +1 more source

STARSPOTS ON WASP-85 [PDF]

open access: yesThe Astronomical Journal, 2016
ABSTRACT By analyzing K2 short-cadence observations, we detect starspots on WASP-85A, the host star of the hot Jupiter WASP-85Ab. The detection of recurring starspot occultation events indicates that the planet’s orbit is aligned with the star’s rotational axis ( λ
T. Močnik   +4 more
openaire   +2 more sources

Differential photometry of EK DRA and 29 DRA [PDF]

open access: yesSerbian Astronomical Journal, 2005
We report on BVR precise photometry of active late-type stars EK DRA and 29 DRA in the spring of 2004. The analysis suggests a reasonable fit with single spot model for both cases in the season as far as the V-curve is concerned.
Zboril M.
doaj   +1 more source

Under-Developed and Under-Utilized Eclipsing Binary Model Capabilities [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2012
Existing but largely unused binary star model capabilities are examined. An easily implemented scheme is parameterization of starspot growth and decay that can stimulate work on outer convection zones and their dynamos.
R. E. Wilson
doaj   +1 more source

ON SUNSPOT AND STARSPOT LIFETIMES [PDF]

open access: yesThe Astrophysical Journal, 2014
We consider the lifetimes of spots on the Sun and other stars from the standpoint of magnetic diffusion. While normal magnetic diffusivity predicts lifetimes of sunspots that are too large by at least two orders of magnitude, turbulent magnetic diffusivity accounts for both the functional form of the solar empirical spot-lifetime relation and for the ...
S. J. Bradshaw, P. Hartigan
openaire   +2 more sources

3D Radiative MHD Simulations of Starspots [PDF]

open access: yesThe Astrophysical Journal, 2020
Abstract There are no direct spatially resolved observations of spots on stars other than the Sun, and starspot properties are inferred indirectly through lightcurves and spectropolarimetric data. We present the first self-consistent 3D radiative MHD computations of starspots on G2V, K0V, and M0V stars, which will help us to better ...
Mayukh Panja   +2 more
openaire   +3 more sources

Joint Modeling of Radial Velocities and Photometry with a Gaussian Process Framework

open access: yesThe Astrophysical Journal, 2023
Developments in the stability of modern spectrographs have led to extremely precise instrumental radial velocity (RV) measurements. For most stars, the detection limit of planetary companions with these instruments is expected to be dominated by ...
Quang H. Tran   +3 more
doaj   +1 more source

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