Spectral Analysis of LMC-X2 with XMM/Newton

Risultato della ricerca: Articlepeer review


We present the results of the analisys of an archival observation of LMC X-2 performed with XMM/Newton. The spectra of this source has never been analyzed with a high precision instrument before. The spectrum of the source can be fitted with a blackbody with a temperature 1.5 keV plus a disk blackbody at 0.8 keV. We argue that the emission of this source can be straightforwardly interpreted as a sum of the emission from a boundary layer between the NS and the disc and a blackbody component coming from the disc itself. The detection of the O VIII emission line (and the lack of detection of lines in the iron region) can be due to the fact that the source lies in the Large Magellanic Cloud.
Lingua originaleEnglish
pagine (da-a)325-329
Numero di pagine5
RivistaChinese Journal of Astronomy and Astrophysics
Stato di pubblicazionePublished - 2008


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