activity
19942003
most citedOn the Evolution and Appearance of a Surviving Companion after a Type Ia Supernova Explosion

15 citations · 15 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph2003

Exploring the Nature of Weak Chandra Sources near the Galactic Centre

R. M. Bandyopadhyay, K. M. Blundell, Ph. Podsiadlowski +5

We present early results from the first IR imaging of the weak X-ray sources discovered in a recent Chandra survey towards the Galactic Centre. From our VLT observations we will id…

astro-ph200315 cited

On the Evolution and Appearance of a Surviving Companion after a Type Ia Supernova Explosion

Philipp Podsiadlowski

One promising method to test progenitor models for Type Ia supernovae is to identify surviving companion stars in historical supernova remnants. A surviving companion will have bee…

astro-ph2001

Cataclysmic Variables with Evolved Secondaries and the Progenitors of AM CVn Stars

Ph. Podsiadlowski, Z. Han, S. Rappaport

We present the results of a systematic study of cataclysmic variables (CVs) and related systems, combining detailed binary-population synthesis (BPS) models with a grid of 120 bina…

astro-ph2001

Common-Envelope Evolution: the Nucleosynthesis in Mergers of Massive Stars

N. Ivanova, Ph. Podsiadlowski, H. Spruit

We study the merging of massive stars inside a common envelope for binary systems consisting of a red supergiant with a mass of 15-20 Msun and a main-sequence companion of 1-5 Msun…

astro-ph1998

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

S. N. Phillips, T. Shahbaz, Ph. Podsiadlowski

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 tre…

astro-ph1994

The Effects of High-Velocity Supernova Kicks on the Orbital Properties and Sky Distributions of Neutron Star Binaries

W. N. Brandt, Ph. Podsiadlowski

We systematically investigate the effects of high supernova kick velocities on the orbital parameters of post-supernova neutron-star binaries. Using Monte- Carlo simulations, we de…