Results 11 to 20 of about 465,086 (299)

A Note on the Flare Stars in the Coalsack [PDF]

open access: yesJournal of Mathematical and Fundamental Sciences, 2019
Ringkasan. Didalam tulisan ini dilaporkan penemuan 5 buah "flare stars" di daerah Coalsack.  Abstract. The discovery of 5 flare stars in the Coalsack is reported. 
B. Hidajat, A. Kuncoro
doaj   +2 more sources

Magnetic Activity of Different Types of Variable Stars Observed by TESS Mission

open access: yesUniverse, 2023
The investigation of the magnetic activity of different types of variable stars holds significant implications for our understanding of the physical processes and evolution of stars.
Ming Zhong   +3 more
doaj   +2 more sources

Evolution of Flare Activity in GKM Stars Younger Than 300 Myr over Five Years of TESS Observations [PDF]

open access: yesThe Astronomical Journal
Stellar flares are short-duration (< hours) bursts of radiation associated with surface magnetic reconnection events. Stellar magnetic activity generally decreases as a function of both the age and Rossby number, R _0 , a measure of the relative ...
Adina D. Feinstein   +4 more
doaj   +3 more sources

Flare Activity and Magnetic Feature Analysis of the Flare Stars. III. K-type Dwarf Binary Components

open access: yesThe Astrophysical Journal
We analyze the light curve of 199 dwarf stars that are members of binary systems resolved by Kepler mission. All of them are K-type active stars in binary systems of which their flare activity has been confirmed.
Hadis Goodarzi   +2 more
doaj   +2 more sources

Temporal Variation of Flare Occurrence Rates via the Spot Evolution on the Sun and Solar-type Stars

open access: yesThe Astrophysical Journal
The spot evolution on the Sun and solar-type stars is important for understanding the nature of consequential flaring activity. This study statistically investigates the variance of flare occurrence rate through the time evolution of spots on the Sun and
Takato Tokuno   +3 more
doaj   +2 more sources

The White-light Superflares from Cool Stars in GWAC Triggers [PDF]

open access: yesThe Astrophysical Journal
M-type stars are the ones that flare most frequently, but how big their maximum flare energy can reach is still unknown. We present 163 flares from 162 individual M2 through L1-type stars that triggered the GWAC, with flare energies ranging from 10 ^32.2
Guang-Wei Li   +18 more
doaj   +2 more sources

A Statistical Study of Soft X-Ray Flares on Solar-type Stars [PDF]

open access: yesThe Astrophysical Journal, 2023
The statistical characteristics of stellar flares at optical bands have received extensive study, but they remain to be studied at soft X-ray bands, in particular for solar-type stars.
Z. H. Zhao   +4 more
doaj   +2 more sources

An “A star” on an M star during a flare within a flare [PDF]

open access: yesProceedings of the International Astronomical Union, 2010
AbstractM dwarfs produce explosive flare emission in the near-UV and optical continuum, and the mechanism responsible for this phenomenon is not well-understood. We present a near-UV/optical flare spectrum from the rise phase of a secondary flare, which occurred during the decay of a much larger flare.
Kowalski, Adam F.   +4 more
openaire   +2 more sources

Flare stars in nearby Galactic open clusters based on TESS data [PDF]

open access: yes, 2021
The study is devoted to search for flare stars among confirmed members of Galactic open clusters using high-cadence photometry from TESS mission. We analyzed 957 high-cadence light curves of members from 136 open clusters.
Bicz, K.   +11 more
core   +1 more source

Spectral Observations of Flare Stars [PDF]

open access: yesSymposium - International Astronomical Union, 1990
Spectral observations of 6 flare stars in the Pleiades cluster are carried out which occupy different positions on the Hertzsprung-Russell diagram relative to the main sequence: above and below it. The spectral indices which are sensible to luminosity or temperature of the star photosphere are determined.
L.V. Mirzoyan   +2 more
openaire   +1 more source

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