Results 51 to 60 of about 2,393 (171)

A Superflare on YZ Canis Minoris Observed by the Seimei Telescope and TESS: Red Asymmetry of Hα Emission Associated with White-light Emission

open access: yesThe Astrophysical Journal, 2023
Active M-type stars are known to often produce superflares on the surface. Radiation from stellar (super)flares is important for exoplanet habitability, but the mechanisms are not well understood.
Keiichi Namizaki   +6 more
doaj   +1 more source

Optical and EUV observations of solar flare kernels [PDF]

open access: yesAstronomy & Astrophysics, 2005
We present high-resolution spectral observations, covering the entire optical region (3800−9000 A), of a solar flare observed during a multiwavelength campaign. The flare, recorded on 2002 January 11, was a medium solar flare event (GOES class C7.5).
García-Alvarez, D.   +5 more
openaire   +2 more sources

ABOUT THE FLASHES’ ACTIVITY OF AO535+26 IN OPTICAL BAND

open access: yesOdessa Astronomical Publications, 2017
After the great multipulse outburst of Oct. 1995 (JD 2450019) was recorded we followed the optical activity of Be/neutron star binary system A0535+26. The  information on optical flares during 25 years of photoelectric observations was replenished by the
N. I. Dorokhov   +2 more
doaj   +1 more source

Shock Cooling and Breakout Emission for Optical Flares Associated with Gravitational-wave Events

open access: yesThe Astrophysical Journal
The astrophysical origin of stellar-mass black hole (BH) mergers discovered through gravitational waves (GWs) is widely debated. Mergers in the disks of active galactic nuclei (AGNs) represent promising environments for at least a fraction of these ...
Hiromichi Tagawa   +4 more
doaj   +1 more source

Magnetic Field Amplification and Blazar Flares

open access: yesEPJ Web of Conferences, 2013
Recent multiwavelength observations of PKS 0208-512 by SMARTS, Fermi, and Swift revealed that γ-ray and optical light curves of this flat spectrum radio quasars are highly correlated, but with an exception of one large optical flare having no ...
Chen Xuhui   +3 more
doaj   +1 more source

AT 2019aalc: A Bowen Fluorescence Flare with a Precursor Flare in an Active Galactic Nucleus

open access: yesThe Astrophysical Journal
AT 2019aalc is a peculiar sequence of highly variable emission events observed towards the nucleus of the broad-line active galactic nucleus (AGN) SDSS J152416.66+045119.0.
Marzena Śniegowska   +12 more
doaj   +1 more source

A circular white-light flare with impulsive and gradual white-light kernels

open access: yesNature Communications, 2017
White-light flares are rare solar events entailing emission in the optical continuum. Here, the authors report a nearly circular white-light flare observed on March 10th 2015 that contains simultaneously both impulsive and gradual white-light kernels.
Q. Hao   +7 more
doaj   +1 more source

Optical variability of the blazar 3C 454.3 during 2007-2010

open access: yesEPJ Web of Conferences, 2013
The optical variability of the blazar 3C 454.3 during 2007-2010 has been studied using the results of multicolor (BVRIJHK) observations. The existence of two variable synchrotron sources was found.
Hagen-Thorn V.A.   +4 more
doaj   +1 more source

Polarization and Spectral Energy Distribution in OJ 287 during the 2016/17 Outbursts

open access: yesGalaxies, 2017
We report optical photometric and polarimetric observations of the blazar OJ 287 gathered during 2016/17. The high level of activity, noticed after the General Relativity Centenary flare, is argued to be part of the follow-up flares that exhibited high ...
Mauri Valtonen   +41 more
doaj   +1 more source

FUMES. IV. Optical and Far-ultraviolet Spectra of a Flare on the M Dwarf GJ 4334

open access: yesThe Astronomical Journal
On 2017 September 20, we observed GJ 4334, an M5V dwarf rotating with a period of 23.5 days, simultaneously with both the Space Telescope Imaging Spectrograph aboard Hubble (1160–1710 Å) and the Dual Imaging Spectrograph mounted on the 3.5 m telescope at
Girish M. Duvvuri   +7 more
doaj   +1 more source

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