Results 31 to 40 of about 17,719 (230)
X-ray flares in Orion young stars. I. Flare characteristics
Pre-main sequence (PMS) stars are known to produce powerful X-ray flares which resemble magnetic reconnection solar flares scaled by factors up to 10^4.
Drake J. J. +13 more
core +1 more source
Swift, XMM-Newton, and NuSTAR observations of PSR J2032+4127/MT91 213 [PDF]
We report our recent Swift, NuSTAR, and XMM-Newton X-ray and Lijiang optical observations on PSR J2032+4127/MT91 213, the gamma-ray binary candidate with a period of 45-50 years.
Hou, X. +5 more
core +2 more sources
The correlation between soft and hard X-rays component in flares: from the Sun to the stars
In this work we study the correlation between the soft (1.6--12.4 keV, mostly thermal) and the hard (20--40 and 60--80 keV, mostly non-thermal) X-ray emission in solar flares up to the most energetic events, spanning about 4 orders of magnitude in peak ...
Favata, F. +3 more
core +1 more source
Continuous heating of a giant X-ray flare on Algol [PDF]
Giant flares can release large amounts of energy within a few days: X-ray emission alone can be up to ten percent of the star's bolometric luminosity.
BH Foing +27 more
core +3 more sources
The X-ray emission from flares on cool (i.e. spectral-type F-M) stars is indicative of very energetic, transient phenomena, associated with energy release via magnetic reconnection. We present a uniform, large-scale survey of X-ray flare emission.
Fyfe, D. +3 more
core +1 more source
X-ray Flaring Activity of Mrk 421 [PDF]
We report results from a systematic search for X-ray flares from Mrk 421, using archival data from the Rossi X-ray Timing Explorer (RXTE) satellite. The flares are clearly seen over a wide range of timescales.
Cui, Wei
core +3 more sources
Flare X-Ray Observations of AB Doradus: Evidence of Stellar Coronal Opacity
13 pages, 3 figures, to be published in ApJ ...
Matranga, M. +3 more
openaire +3 more sources
X-Ray flares in Orion Young Stars. II. Flares, Magnetospheres, and Protoplanetary Disks
We study the properties of powerful X-ray flares from 161 pre-main sequence (PMS) stars observed with the Chandra X-ray Observatory in the Orion Nebula region.
Alef W. +21 more
core +1 more source
Probing clumpy stellar winds with a neutron star [PDF]
INTEGRAL, the European Space Agency's gamma-ray observatory, tripled the number of super-giant high-mass X-ray binaries (sgHMXB) known in the Galaxy by revealing absorbed and fast transient (SFXT) systems.
Heras, J. Zurita, Walter, R.
core +2 more sources
Was an Outburst of Aquila X-1 a Magnetic Flare?
I point to an interesting similarity in the radio and the soft X-ray light curves between the November 2009 outburst of the X-ray binary Aquila X-1 and some solar flares.
Benz +19 more
core +1 more source

