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Modeling X-Ray Emission of a Straight Jet:. PKS 0920-397
DOI: 10.1142/S0218271810017147 Bibcode: 2010IJMPD..19..879S

Siemiginowska, A.; Birkinshaw, M.; Worrall, D. M. +14 more

We summarize a study of PKS 0920-397 using our 42 ks Chandra observation in conjunction with our ATCA 20GHz image, and HST/ACS F814W and F475W images. We investigate the hypothesis that the jet X-ray emission is due to inverse-Compton (IC) scattering on the cosmic microwave background (CMB) from the same population of relativistic electrons that g…

2010 International Journal of Modern Physics D
eHST 2
Counterpart Candidates to the Unidentified Fermi Source 0FGL J1848.6-0138
DOI: 10.1142/S0218271810016695 Bibcode: 2010IJMPD..19..825L

Combi, J. A.; Luque-Escamilla, P. L.; Martí, J. +3 more

Here we report the finding of a few counterpart candidates inside the 95% confidence error box of the Fermi LAT unidentified gamma-ray source 0FGL J1848.6-0138. Among them, the globular cluster GLIMPSE-C01 is specially remarkable. It offers a conceivable physical scenario for gamma-ray production and if confirmed to be counterpart it would be the …

2010 International Journal of Modern Physics D
XMM-Newton 1
Pulse Characterization of GRBs with Known Redshift
DOI: 10.1142/S0218271810016798 Bibcode: 2010IJMPD..19..997V

Kawai, Nobuyuki; Vasquez, Nicolas

Gamma-ray Bursts (GRBs) are one of the most promising tools in the study of cosmology. The luminosity, energy, light curve parameters and spectral measures could yield to the calibration of standard candles in the Universe. Nevertheless, cosmological and non-cosmological effects are not well understood. Aiming to clarify the possible effects, we s…

2010 International Journal of Modern Physics D
Suzaku 1
X-Ray and Gamma-Ray Observations of the Inner Region of Mgro J2019+37
DOI: 10.1142/S0218271810016816 Bibcode: 2010IJMPD..19..811Z

Paredes, J. M.; Zabalza, V.

In order to better understand the puzzling extended TeV source MGRO J2019+37, we have performed a multiwavelength campaign from radio to X-ray covering most of its extent. Here we present an X-ray mosaic including a new observation and two archival observations performed by the X-ray observatory XMM-Newton. We have also observed the source with th…

2010 International Journal of Modern Physics D
XMM-Newton 1