Dirk Pandel

Publication List Details

Period

2000 - 2008

Number

8

Co-Authors

Relativistic Iron Line Emission from the Neutron Star Low-mass X-ray Binary 4U 1636-536 (2008)

Pandel, Dirk, Kaaret, Philip, Corbel, Stephane

We present an analysis of XMM-Newton and RXTE data from three observations of the neutron star LMXB 4U 1636-536. The X-ray spectra show clear evidence of a broad, asymmetric iron emission line...

X-ray Observations of the Boundary Layer in Dwarf Novae at Low Accretion Rates (2005)

Pandel, Dirk, Cordova, France A., Mason, Keith O., Priedhorsky, William C.

We present a spectral analysis of XMM-Newton data of ten dwarf novae, nine of which were observed during a quiescent state. The X-ray spectra indicate the presence of a hot, optically thin plasma...

Irregular Mass Transfer in the Polars VV Puppis and V393 Pavonis during the Low State (2005)

Pandel, Dirk, Cordova, France A.

The polars VV Pup and V393 Pav were observed with XMM-Newton during states of low accretion rate with peak X-ray luminosities of ~1 x 10^30 and ~1 x 10^31 erg/s, respectively. In both polars,...

X-ray and UV observations of the dwarf nova VW Hyi in quiescence (2003)

Pandel, Dirk, Cordova, France A., Howell, Steve B.

We present an analysis of X-ray and ultra-violet data of the dwarf nova VW Hyi that were obtained with XMM-Newton during the quiescent state. The X-ray spectrum indicates the presence of an optically...

XMM-Newton observes flaring in the polar UZ For during a low state (2002)

Pandel, Dirk, Cordova, France A.

During an XMM-Newton observation, the eclipsing polar UZ For was found in a peculiar state with an extremely low X-ray luminosity and occasional X-ray and UV flaring. For most of the observation, UZ...

First XMM-Newton observations of strongly magnetic cataclysmic variables - II. Timing studies of DP Leo and WW Hor (2001)

Pandel, Dirk, Cordova, France A., Shirey, Robert E., Ramsay, Gavin, Cropper, Mark, Mason, Keith O., ...

XMM-Newton was used to observe two eclipsing, magnetic cataclysmic variables, DP Leo and WW Hor, continuously for three orbital cycles each. Both systems were in an intermediate state of accretion....

First XMM-Newton observations of a cataclysmic variable II: the X-ray spectrum of OY Car (2000)

Ramsay, Gavin, Cordova, France, Cottam, Jean, Mason, Keith, Much, Rudi, Osborne, Julian, ...

We present XMM-Newton X-ray spectra of the disc accreting cataclysmic variable OY Car, which were obtained during the performance verification phase of the mission. These data were taken 4 days after...

First XMM-Newton observations of a Cataclysmic Variable I: Timing studies of OY Car (2000)

Ramsay, Gavin, Poole, Tracey, Mason, Keith, Cordova, France, Priedhorsky, William, Breeveld, Alice, ...

We present XMM-Newton observations of the eclipsing, disc accreting, cataclysmic variable OY Car which were obtained as part of the performance verification phase of the mission. The star was...