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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Philipp Podsiadlowski

Emeriti Professor

Sub department

  • Astrophysics
philipp.podsiadlowski@seh.ox.ac.uk
Denys Wilkinson Building
  • About
  • Publications

Episodic mass ejections from common-envelope objects

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 470:2 (2017) 1788-1808

Authors:

M Clayton, P Podsiadlowski, N Ivanova, S Justham

A common-envelope wind model for Type Ia supernovae - I. Binary evolution and birth rate

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 469:4 (2017) 4763-4787

Authors:

X Meng, P Podsiadlowski

Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity

ASTRONOMY & ASTROPHYSICS 604 (2017) ARTN A55

Authors:

P Marchant, N Langer, P Podsiadlowski, TM Tauris, S de Mink, I Mandel, TJ Moriya

Stellar winds in massive X-ray binaries

Proceedings of the International Astronomical Union Cambridge University Press 12:S329 (2017) 355-358

Authors:

P Kretschmar, S Mart铆nez-N煤帽ez, E Bozzo, LM Oskinova, J Puls, L Sidoli, JO Sundqvist, P Blay, M Falanga, F F眉rst, A G铆menez-Garc铆a, I Kreykenbohm, M K眉hnel, A Sander, JM Torrej贸n, J Wilms, Philipp Podsiadlowski, A Manousakis

Abstract:

Strong winds from massive stars are a topic of interest to a wide range of astrophysical fields. In High-Mass X-ray Binaries the presence of an accreting compact object on the one side allows to infer wind parameters from studies of the varying properties of the emitted X-rays; but on the other side the accretor's gravity and ionizing radiation can strongly influence the wind flow. Based on a collaborative effort of astronomers both from the stellar wind and the X-ray community, this presentation attempts to review our current state of knowledge and indicate avenues for future progress.

Light-curve and spectral properties of ultrastripped core-collapse supernovae leading to binary neutron stars

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 466:2 (2017) 2085-2098

Authors:

TJ Moriya, PA Mazzali, N Tominaga, S Hachinger, SI Blinnikov, TM Tauris, K Takahashi, M Tanaka, N Langer, P Podsiadlowski

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