Philipp Podsiadlowski: Publications

Cygnus X-2: The descendant of an intermediate-mass X-ray binary

ASTROPHYSICAL JOURNAL 529:2 (2000) 946-951

Authors:

P Podsiadlowski, S Rappaport

The outburst radial velocity curve of X-Ray Nova Scorpii 1994 (=GRO J1655--40)

Monthly Notices of the Royal Astronomical Society Blackwell Publishing Inc. (1999)

Authors:

SN Phillips, T Shahbaz, P Podsiadlowski

Abstract:

We present a reanalysis of the outburst radial velocity data for X-Ray Nova Scorpii 1994. Using a model based on X-ray heating of the secondary star we suggest a more realistic treatment of the radial velocity data. Solutions are obtained in the (K_2,q) plane which, when combined with the published value for the binary mass ratio and inclination, constrain the mass of the black hole to within the region 4.1

The outburst radial velocity curve of X-ray Nova Scorpii 1994 (= GRO J1655-40): a reduced mass for the black hole?

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 304:4 (1999) 839-844

Authors:

SN Phillips, T Shahbaz, P Podsiadlowski

Presupernova evolution in massive binaries

NATO ADV SCI INST SE 477 (1996) 181-200

Authors:

P Podsiadlowski, PC Joss, OR Pols, WN Brandt

The progenitors of hydrogen-deficient supernovae

ASTR SOC P 96 (1996) 419-432

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