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Solar Neighborhood Flare Stars – a Review [PDF]
Symposium - International Astronomical Union, 1975 Since Gershberg's (1970a) very thorough review of the subject, numerous papers dealing with the collective properties of flare stars have appeared (Petit, 1970; Kunkel, 1970d, 1973; Ambartsumian and Mirzoyan, 1971; Gurzadyan, 1971; Oskanian and Terebizh, 1971a, b; Gershberg, 1972; Veeder, 1973).
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Analysis of the Stellar Occultations during the Unprecedented Long-duration Flare
The Astrophysical Journal LettersIn strong stellar and solar flares, flare loops typically appear during the decay phase, providing an additional contribution to the flare emission and, possibly, obscuring the flare emission.
K. Bicz +4 more
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Optical Spectroscopy of a Flare on Barnard’s Star
Publications of the Astronomical Society of the Pacific, 2006 Accepted for publication in ...
Paulson, D. +5 more
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The Astrophysical JournalStellar eruptive events, such as flares and coronal mass ejections (CMEs), can affect planetary habitability by disturbing the stability of their atmospheres.
Nuri Park +2 more
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Molecular Hydrogen Controls the Temperatures of Flares on TRAPPIST-1
The Astrophysical Journal LettersEarly JWST observations of TRAPPIST-1 have revealed an unexpected puzzle: energetic white-light flares ( E > 10 ^30 erg) reach temperatures of only ∼3500–4000 K, nearly 3 times cooler than typical solar flares, which peak around 9000–10,000 K.
A. I. Shapiro +9 more
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Flare Activity Among Nearby Stars [PDF]
International Astronomical Union Colloquium, 1995 I selected the common objects from our Data Base on 234 UV Cet Flare Stars and Related Objects and the Third Catalogue of Nearby Stars by Gliese & Jahreiss (CNS-3). It is found that manifestation of flare activity (FA) (flares in any spectral region or photometric variability caused by spots) is observed on 143 flare stars (FS) out of the 3803 CNS ...
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Time-dependent Stellar Flare Models of Deep Atmospheric Heating
The Astrophysical JournalOptical flares have been observed from magnetically active stars for many decades; unsurprisingly, the spectra and temporal evolution are complicated.
Adam F. Kowalski +2 more
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Multiple Generation Star Formation in Cepheus Flare
The Astronomical JournalWe present an analysis of the young stellar moving group ASCC 127 using Gaia DR3 data, significantly expanding its membership to 3971 stars—double the number identified in previous studies.
Fan Wang +10 more
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Magnetic Activity in M-type Stars Based on LAMOST DR11 and TESS Observations
The Astrophysical Journal Supplement SeriesWe have used 898,351 M-type stellar spectra released by Large Sky Area Multi-Object Fiber Spectroscopic Telescope DR11 to calculate the equivalent width of the Ca II infrared triplet (IRT) lines, the residual chromospheric emission, and the parameter ${R}
Linfeng Ren +6 more
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The Astrophysical Journal, 1991 Fourteen cases of flares reported on Mira type stars have been collected. These flares typically have an amplitude of over half a magnitude, a rise time of minutes, and a duration of tens of minutes. Nine of the 11 stars represent a normal cross section of the Mira population, while the remaining two are in symbiotic systems (CH Cyg and RX Pup).
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