activity
20012012
most citedTwo new Intermediate Polars with a soft X-ray component

53 citations · 143 across the 6 of their papers we have counts for

collaborators

6 papers

physics.space-ph2012

The peculiar source XSS J12270-4859: a LMXB detected by FERMI ?

J. M. Bonnet-Bidaud, D. de Martino, M. Mouchet +5

The X-ray source XSS J12270-4859 has been first suggested to be a magnetic cataclysmic variable of Intermediate Polar type on the basis of its optical spectrum and a possible 860 s…

astro-ph2008★ 53 cited

Two new Intermediate Polars with a soft X-ray component

G. Anzolin, D. de Martino, J. -M. Bonnet-Bidaud +4

We analyze the first X-ray observations with XMM-Newton of RXS J070407.9+262501 and 1RXS 180340.0+401214, in order to characterize their broad-band temporal and spectral properties…

astro-ph2008★ 36 cited

1RXSJ173021.5-055933: a cataclysmic variable with a fast-spinning magnetic white dwarf

D. de Martino, G. Matt, K. Mukai +8

We present the first X-ray observations with the XMM-Newton and INTEGRAL satellites of the recently discovered cataclysmic variable 1RXSJ173021.5-055933, together with simultaneous…

astro-ph2006★ 30 cited

The X-ray properties of the magnetic Cataclysmic Variable UU Col

D. de Martino, G. Matt, K. Mukai +5

XMM-Newton observations aimed at determining for the first time the broad-band X-ray properties of the faint high galactic latitude Intermediate Polar UU Col are presented. We perf…

astro-ph2001

A white dwarf with a low magnetic field in the IP RXJ0028.8+5917/V709Cas

J. M. Bonnet-Bidaud, M. Mouchet, D. de Martino +2

We report the first detailed spectroscopic observations of the recently identified intermediate polar RXJ0028.8+5917/V709 Cas. We discovered that the system shows significant EW ~…

astro-ph2001★ 24 cited

The white dwarf revealed in the intermediate polar V709 Cassiopeiae

J. M. Bonnet-Bidaud, M. Mouchet, D. de Martino +2

Results are presented from the first detailed spectroscopic observations of the recently identified intermediate polar RXJ0028.8+5917/V709 Cas. The study of the emission line radia…