414 research outputs found
Gamma-ray bursts and X-ray melting of material as a potential source of chondrules and planets
The intense radiation from a gamma-ray burst (GRB) is shown to be capable of
melting stony material at distances up to 300 light years which subsequently
cool to form chondrules. These conditions were created in the laboratory for
the first time when millimeter sized pellets were placed in a vacuum chamber in
the white synchrotron beam at the European Synchrotron Radiation Facility
(ESRF). The pellets were rapidly heated in the X-ray and gamma-ray furnace to
above 1400 C melted and cooled. This process heats from the inside unlike
normal furnaces. The melted spherical samples were examined with a range of
techniques and found to have microstructural properties similar to the
chondrules that come from meteorites. This experiment demonstrates that GRBs
can melt precursor material to form chondrules that may subsequently influence
the formation of planets. This work extends the field of laboratory
astrophysics to include high power synchrotron sources.Comment: 8 pages, 10 figures. Proceedings of the 5th INTEGRAL Workshop, Munich
16-20 February 2004. High resolution figures available at
http://bermuda.ucd.ie/%7Esmcbreen/papers/duggan_01.pd
Gamma-ray bursts and X-ray melting of material to form chondrules and planets
Chondrules are millimeter sized objects of spherical to irregular shape that
constitute the major component of chondritic meteorites that originate in the
region between Mars and Jupiter and which fall to Earth. They appear to have
solidified rapidly from molten or partially molten drops. The heat source that
melted the chondrules remains uncertain. The intense radiation from a gamma-ray
burst (GRB) is capable of melting material at distances up to 300 light years.
These conditions were created in the laboratory for the first time when
millimeter sized pellets were placed in a vacuum chamber in the white
synchrotron beam at the European Synchrotron Radiation Facility. The pellets
were rapidly heated in the X-ray and gamma-ray furnace to above 1400C melted
and cooled. This process heats from the inside unlike normal furnaces. The
melted spherical samples were examined with a range of techniques and found to
have microstructural properties similar to the chondrules that come from
meteorites. This experiment demonstrates that GRBs can melt precursor material
to form chondrules that may subsequently influence the formation of planets.
This work extends the field of laboratory astrophysics to include high power
synchrotron sources.Comment: 4 pages, 4 figures. Full resolution figures available from A&
Very High Energy gamma-rays from electron/positron Pair Halos
In this paper we study the formation of giant electrons-positron pair halos
around the powerful high energy extragalactic sources. We investigate the
dependence of radiation of pair halos, in particular the spectral and angular
distributions on the energy spectrum of the primary gamma-rays, the redshift of
the source, and the flux of the extragalactic background light.Comment: 17 pages, 17 figures, published in Volume No. 18, Issue No. 06 of
"International Journal Of Modern Physics D
The frontier of darkness: the cases of GRB 040223, GRB 040422, GRB 040624
Understanding the reasons for the faintness of the optical/near-infrared
afterglows of the so-called dark bursts is essential to assess whether they
form a subclass of GRBs, and hence for the use of GRBs in cosmology. With VLT
and other ground-based telescopes, we searched for the afterglows of the
INTEGRAL bursts GRB 040223, GRB 040422 and GRB 040624 in the first hours after
the triggers. A detection of a faint afterglow and of the host galaxy in the K
band was achieved for GRB 040422, while only upper limits were obtained for GRB
040223 and GRB 040624, although in the former case the X-ray afterglow was
observed. A comparison with the magnitudes of a sample of afterglows clearly
shows the faintness of these bursts, which are good examples of a population
that an increasing usage of large diameter telescopes is beginning to unveil.Comment: 4 pages, 2 figures. To appear in the proceedings of the 16th Annual
October Astrophysics Conference in Maryland "Gamma Ray Bursts in the Swift
Era", eds. S. Holt, N. Gehrels & J. Nouse
The bright optical/NIR afterglow of the faint GRB 080710 - Evidence for a jet viewed off axis
We investigate the optical/near-infrared light curve of the afterglow of GRB
080710 in the context of rising afterglows. Optical and near-infrared
photometry was performed using the seven channel imager GROND and the
Tautenburg Schmidt telescope. X-ray data were provided by the X-ray Telescope
onboard the Swift satellite. The optical/NIR light curve of the afterglow of
GRB 080710 is dominated by an initial increase in brightness, which smoothly
turns over into a shallow power law decay. The initially rising achromatic
light curve of the afterglow of GRB 080710 can be accounted for with a model of
a burst viewed off-axis or a single jet in its pre deceleration phase and in an
on-axis geometry. An unified picture of the afterglow light curve and prompt
emission properties can be obtained with an off-axis geometry, suggesting that
late and shallow rising optical light curves of GRB afterglows might be
produced by geometric effects.Comment: 9 pages, 4 figures, accepted by A and
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