Results 51 to 60 of about 904 (176)
Starspot Imaging Using VRI Photometry [PDF]
Recent progress on maximum-entropy imaging of stellar surface brightness distributions using VRI photometry and Doppler-broadened absorption line profiles is reported. VRI photometry generally provides tighter constraints on starspot configurations than does Doppler imaging (which requires the use of large telescopes).
openaire +1 more source
A Flexible Model for Investigating the Properties of Starspots: Model Characterization
Starspots are sites of intense magnetic fields near a star’s optical surface that actively suppress convective flows causing the area to be dimmer and cooler than the surrounding ambient photosphere.
Ash, Amanda +5 more
core +1 more source
Magnetic activity on the young Sun: A case study of EK Draconis
Context. Young solar analog stars provide key insights into the early stages of stellar evolution, particularly in terms of magnetic activity and rotation.
Görgei A. +10 more
doaj +1 more source
Doppler imaging combined with high-cadence photometry
Context. Latitude distribution of stellar magnetic activity is not well constrained by observations, despite its importance for a better understanding of stellar dynamos and their effects on planetary environments. Aims.
Lee S. +13 more
doaj +1 more source
Core-envelope Decoupling Drives Radial Shear Dynamos in Cool Stars
Differential rotation is thought to be responsible for the dynamo process in stars like our Sun, driving magnetic activity and starspots. We report that starspot measurements in the Praesepe open cluster are strongly enhanced only for stars that depart ...
Lyra Cao +2 more
doaj +1 more source
Starspots on late-type stars and their correlation with flare activity
Recent space-based observations (e.g., Kepler mission) found thousands of ``superflares’’ on G-, K-, and M-type stars. These superflare stars show quasi-periodic brightness variations caused by the rotation of the star with starspots.
Honda, Satoshi (5266576) +15 more
core +1 more source
Forward modeling solar spectra onto Doppler images of λ And
Context. Due to their high chromospheric activity and photometric variability, RS CVn-type binaries are ideal laboratories for studying stellar surface structures and the corresponding stellar activity relations.
Adebali Ö., Pietrow A. G. M.
doaj +1 more source
Stellar Flares, Superflares, and Coronal Mass Ejections—Entering the Big Data Era
Flares, sometimes accompanied by coronal mass ejections (CMEs), are the result of sudden changes in the magnetic field of stars with high energy release through magnetic reconnection, which can be observed across a wide range of the electromagnetic ...
Krisztián Vida +8 more
doaj +1 more source
Subduction, Stratosphere, Starspots, and Sushi
Highlights from AGU’s joint meeting with the Japan Geophysical Union.
Jenny Lunn +4 more
openaire +1 more source
Starspots on the active young solar-type star AH Lep
Young solar-type stars inform us about the early evolution of objects that form a major component of the stellar population of our galaxy. Single active young solar-type stars close to the Sun’s mass also provide us with proxies for the Sun’s early ...
Treschman, Keith
core

