activity
19972026
most citedThe eROSITA X-ray telescope on SRG

884 citations · 6.5k across the 220 of their papers we have counts for

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Showing 2000Show all

6 papers · 1 filter

astro-ph2000★ 9 cited

X-ray emission in the direction of the SNR G318.2+0.1

F. Bocchino, A. N. Parmar, S. Mereghetti +3

We report the discovery of three X-ray sources within the radio shell G318.2+0.1, one of which may be extended. Two of the sources were detected during the \sax Galactic Plane Surv…

astro-ph2000★ 123 cited

Broad band spectrum of Cygnus X-1 in two spectral states with BeppoSAX

F. Frontera, E. Palazzi, A. A. Zdziarski +13

We report on the 0.5--200 keV spectral properties of Cyg X-1 observed at different epochs with the Narrow Field Instruments of the BeppoSAX satellite. The source was in its soft st…

astro-ph2000★ 2 cited

ASCA and BeppoSAX observations of the peculiar X-ray source 4U1700+24/HD154791

D. Dal Fiume, N. Masetti, C. Bartolini +9

The X-ray source 4U1700+24/HD154791 is one of the few galactic sources whose counterpart is an evolved M star. In X-rays the source shows extreme erratic variability and a complex…

astro-ph2000★ 3 cited

Cyclotron lines in X-ray pulsars as a probe of relativistic plasmas in superstrong magnetic fields

D. Dal Fiume, Filippo Frontera, Nicola Masetti +7

The systematic search for the presence of cyclotron lines in the spectra of accreting X-ray pulsars is being carried on with the BeppoSAX satellite since the beginning of the missi…

astro-ph2000★ 1 cited

X-ray/optical observations of XTE J0421+560/CI Cam in quiescence

M. Orlandini, A. N. Parmar, F. Frontera +8

We report on a BeppoSAX observation of the transient X-ray source XTE J0421+560 during quiescence performed ~150 days after the 1998 April outburst. The source had an unabsorbed 0.…

astro-ph2000★ 3 cited

Broad-band BeppoSAX observation of the low-mass X-ray binary X1822-371

A. N. Parmar, T. Oosterbroek, S. Del Sordo +4

Results of a 1997 September 9-10 BeppoSAX observation of the 5.57 hr low-mass X-ray binary (LMXRB) X1822-371 are presented. The 0.3-40 keV spectrum is unusually complex and cannot…