activity
19982009
most citedLatest results on Jovian disk X-rays from XMM-Newton

55 citations · 216 across the 15 of their papers we have counts for

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Showing 2004 · astro-phShow all

10 papers · 2 filters

astro-ph2004

Geometrical constraints upon the unipolar model of V407 Vul and RXJ0806.3+1527

S. C. C. Barros, T. R. Marsh, P. Groot +5

V407 Vul and RX J0806.3+1527 are X-ray emitting stars with X-ray light curves that are 100% modulated on periods of 569 and 321 seconds respectively. These periods and no others ar…

astro-ph2004

XMM-Newton observations of the ultra-compact binary RX J1914+24

Gavin Ramsay, Pasi Hakala, Kinwah Wu +4

We present XMM-Newton observations of the 569 sec period system RX J1914+24 (V407 Vul). This period is believed to represent the binary orbital period making it an ultra-compact bi…

astro-ph2004

XMM-Newton observations of UW CrB -- detection of X-ray bursts and evidence for accretion disc evolution

P. Hakala, G. Ramsay, P. Muhli +4

UW CrB (MS1603+2600) is a peculiar short period X-ray binary that exhibits extraordinary optical behaviour. The optical light curve shape of the system changes drastically from nig…

astro-ph2004

Properties of serendipitous X-ray flares discovered in XMM-Newton observations

Duncan Trenholme, Gavin Ramsay, Carl Foley

We present the results of a search of the XMM-Newton public data archive for stellar X-ray flares. We find eight flaring sources for which we identify 7 optical counterparts. Three…

astro-ph2004

XMM-Newton observations of the eclipsing polar EP Dra

Gavin Ramsay, C. M. Bridge, Mark Cropper +3

We present XMM-Newton observations of the eclipsing polar EP Dra which cover nearly 3 binary orbital cycles. The X-ray and UV data show evidence for a prominent dip before the ecli…

astro-ph2004

First observation of Jupiter by XMM-Newton

G. Branduardi-Raymont, R. F. Elsner, G. R. Gladstone +4

We present the first X-ray observation of Jupiter by XMM-Newton. Images taken with the EPIC cameras show prominent emission, essentially all confined to the 0.2-2.0 keV band, from…