Investigation of flare stars in the pleiades by the method of stellar tracks. I

Astrophysics ◽  
1999 ◽  
Vol 42 (3) ◽  
pp. 264-269
Author(s):  
H. S. Chavushian ◽  
G. H. Broutian ◽  
A. V. Oskanian
Keyword(s):  
Flare Stars

A Search for Microflaring Activity on dMe Flare Stars. II. Observations of YZ Canis Minoris

1999 ◽  
Vol 516 (2) ◽  
pp. 916-923 ◽  
Author(s):  
R. D. Robinson ◽  
K. G. Carpenter ◽  
J. W. Percival
Keyword(s):  
Flare Stars

scholarly journals A combined radio and optical study of flare stars. The long-duration events

1979 ◽  
Vol 187 (3) ◽  
pp. 405-419 ◽  
Author(s):  
G. J. Nelson ◽  
R. D. Robinson ◽  
O. B. Slee ◽  
G. Fielding ◽  
A. A. Page ◽  
...  
Keyword(s):  
Optical Study ◽  
Long Duration ◽  
Flare Stars

Microwave observations of flare stars UV Ceti, at mic, and AU mic

2008 ◽  
pp. 284-286
Author(s):  
M. R. Kundu ◽  
P. D. Jackson ◽  
M. Melozzi ◽  
S. M. White
Keyword(s):  
Flare Stars

A VLA survey of dMe flare stars

2008 ◽  
pp. 103-105 ◽  
Author(s):  
P. D. Jackson ◽  
M. R. Kundu ◽  
S. M. White
Keyword(s):  
Flare Stars

scholarly journals Double-Peaked Flare Events on red Dwarf Stars and Solar ‘Sympathetic’ Flares

1976 ◽  
Vol 71 ◽  
pp. 475-475
Author(s):  
M. Rodonò
Keyword(s):  
Proximity Effect ◽  
Binary Systems ◽  
Angular Separation ◽  
Dwarf Stars ◽  
Multiple Systems ◽  
Photometric Observations ◽  
Red Dwarfs ◽  
Flare Stars ◽  
Red Dwarf Stars ◽  
The Individual

About 50% of the flare events observed on red dwarfs are at least double-peaked. As the majority of flare stars are members of double or multiple systems, the possibility that time-overlapping flares originate quasi-simultaneously on the individual components is discussed.Assuming a poissonian occurrence of flares in both components, the expected probability of observing double-peaked flares is lower than 1% for the most active binary systems.However, from photometric observations of the double flare star EQ Peg (BD +19°5116 AB) carried out by the author with an area scanner (the components' angular separation is 3.7″) about 20% of the observed flares have been found to be double-peaked flares resulting from separate flares, one in each component. A direct flare triggering of the following flare by the preceding one can be ruled out since the light travel-time between the two components is 3.5 h, while the observed time delay between the flare peaks is about 10 min. Moreover, the proximity effect does not seem to play an important triggering role.It is concluded that, although the analogy with solar ‘sympathetic’ flares is not always applicable, it is the most promising framework within which the majority of double-peaked flare events on red dwarfs must be interpreted.

Emission stars in Cyg OB7. new flare stars. III

Astrophysics ◽  
2011 ◽  
Vol 54 (3) ◽  
pp. 377-383 ◽  
Author(s):  
N. D. Melikian ◽  
V. S. Tamazian ◽  
A. A. Karapetian ◽  
A. L. Samsonyan
Keyword(s):  
Flare Stars ◽  
Emission Stars

scholarly journals Rapid spike flares on AD Leo and EV Lac

1990 ◽  
Vol 137 ◽  
pp. 27-30
Author(s):  
K. P. Panov ◽  
M. S. Ivanova ◽  
A. Antov
Keyword(s):  
Astronomical Observatory ◽  
Monitoring Time ◽  
Flare Stars ◽  
Ev Lac

Photoelectric U - band observations of the flare stars A Leo and EV Lac during the last 9 years obtained at the Bulgarian National Astronomical Observatory revealed 8 rapid spike flares on AD Leo and 9 rapid spike flares on EV Lac which duration is less than 6 seconds. The corresponding total monitoring time is 173.6 hours for AD Leo and 173.3 hours for EV Lac.

scholarly journals Flare Stars in the Orion Nebula

1966 ◽  
Vol 12 (2) ◽  
pp. 454-455
Author(s):  
G. Haro
Keyword(s):  
Orion Nebula ◽  
Flare Stars

scholarly journals Flare stars in nearby Galactic open clusters based on TESS data

2021 ◽  
Vol 51 (1) ◽  
Author(s):  
O. Maryeva ◽  
K. Bicz ◽  
C. Xia ◽  
M. Baratella ◽  
P. Čechvala ◽  
...  
Keyword(s):  
Open Clusters ◽  
Flare Stars
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