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pro vyhledávání: '"Y. Pekon"'
Autor:
Y. Pekon, Solen Balman
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 411:1177-1196
We present the orbital phase-resolved spectra of an intermediate polar, EX Hya, together with the spin phase-resolved spectra during two different epochs using the X-ray Multi-Mirror Mission (XMM–Newton), European Photon Imaging Camera (pn instrume
Autor:
Solen Balman, Y. Pekon
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 388:921-926
We present the Chandra ACIS-S3 data of the old classical nova RR Pic (1925). The source has a count rate of 0.067 ± 0.002 count s -1 in the 0.3-5.0 keV energy range. We detect the orbital period of the underlying binary system in the X-ray wavelengt
Autor:
Solen Balman, Y. Pekon
Publikováno v:
Proceedings of the International Astronomical Union. 7:124-125
We reanalyze a selection of the XMM-Newton RGS (Reflection Grating Spectrometer) data of two classical novae; V4743 Sgr and V2491 Cyg. The high resolution nova spectra in the X-ray wavelengths show existence of absorption features (e.g., blue shifted
ORBITAL-PHASE-RESOLVED SPECTROSCOPY OF THE INTERMEDIATE POLAR FO AQR USINGXMM-NEWTONOBSERVATORY DATA
Autor:
Y. Pekon, Solen Balman
Publikováno v:
The Astronomical Journal. 144:53
We present the orbital-phase-resolved analysis of an archival FO Aqr observation obtained using the X-ray Multi-Mirror Mission, European Photon Imaging Camera (pn instrument). We investigate the variation of the spin pulse amplitudes over the orbital