Results 81 to 90 of about 4,300 (180)

Magnetohydrostatic equilibrium in starspots: dependences on color (T_{eff}) and surface gravity (g)

open access: yes, 2010
Temperature contrasts and magnetic field strengths of sunspot umbrae broadly follow the thermal-magnetic relationship obtained from magnetohydrostatic equilibrium.
Cox   +4 more
core   +1 more source

Sunspots, Starspots, and Elemental Abundances

open access: yesThe Astrophysical Journal, 2017
Abstract Element abundances in the solar photosphere, chromosphere, transition region, and corona are key parameters for investigating sources of the solar wind and for estimating radiative losses in the quiet corona and in dynamical events such as solar flares.
G. A. Doschek, H. P. Warren
openaire   +1 more source

Spectral Biases, Starspot Morphology, and Dynamo Transitions on the Pre-main Sequence: Insights from the X-Shooter WTTS Library

open access: yesThe Astrophysical Journal
Starspots are ubiquitous in young, low-mass stars, yet their impact on the spectral classification and fundamental parameter inference of pre-main-sequence stars (PMS) has been largely overlooked.
Facundo Pérez Paolino   +4 more
doaj   +1 more source

Characterisation of starspot structure and differential rotation of Kepler-411

open access: yesAstronomy & Astrophysics
Context. Starspots and their movements on stellar surfaces enable the mechanisms of stellar magnetic activity to be investigated. Information on the spot distribution and differential rotation provide important constraints for the behaviour of stellar ...
Tuomi Mikko   +2 more
doaj   +1 more source

SS Cygni Revisited

open access: yesActa Polytechnica CTU Proceedings, 2015
New spectroscopic and photometric observations of SS Cygni, the brightest dwarf nova system, have been obtained, with the aim of mapping starspots on the surface of the secondary star.
R. C. Smith   +3 more
doaj   +1 more source

Analysis of new high-precision transit light curves of WASP-10 b: starspot occultations, small planetary radius, and high metallicity

open access: yes, 2011
The WASP-10 planetary system is intriguing because different values of radius have been reported for its transiting exoplanet. The host star exhibits activity in terms of photometric variability, which is caused by the rotational modulation of the spots.
Baraffe   +57 more
core   +1 more source

Starspots: signatures of stellar magnetic activity [PDF]

open access: yesProceedings of the International Astronomical Union, 2008
AbstractStarspots, just as Sunspots, are among the most obvious tracers and signatures of stellar surface magnetic activity. Emphasized already several decades ago as the origin for the rotationally modulated brightness of cool late-type stars, it is just now that we start to trace individual surface features in great enough detail to understand their ...
openaire   +1 more source

Starspot Distribution and Flare Events in Two Young Low-mass Stars Using TESS Data

open access: yesThe Astrophysical Journal
Wide-field high-precision photometric observations such as the Transiting Exoplanet Survey Satellite (TESS) allowed the investigation of the stellar magnetic activity of cool stars. M dwarf starspots and stellar flares are the main indicators of magnetic
Rajib Kumbhakar   +3 more
doaj   +1 more source

What we don't know about starspots [PDF]

open access: yesSymposium - International Astronomical Union, 1996
The scope of this paper will be starspots, and by that I mean regions cooler than the surrounding photosphere (like sunspots) but I also mean the whole range from very small (like sunspots) to very large (such as seen on very active stars like RS CVn).
openaire   +1 more source

Further Study of Starspot Activity and Measurement of Differential Rotation for SZ Piscium

open access: yesThe Astrophysical Journal
We present a series of nine Doppler images of the magnetically active K component of the RS CVn-type binary SZ Piscium (SZ Psc), based on high-resolution spectroscopic data collected from 2014 to 2018.
Yue Xiang   +4 more
doaj   +1 more source

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