activity
19942023
most citedCommon Envelope Evolution: Where we stand and how we can move forward

1k citations · 17.7k across the 141 of their papers we have counts for

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Showing 2005Show all

9 papers · 1 filter

astro-ph2005★ 95 cited

Magnetic Braking of Ap/Bp Stars: Application to Compact Black-Hole X-Ray Binaries

S. Justham, S. Rappaport, Ph. Podsiadlowski

We examine the proposal that the subset of neutron-star and black-hole X-ray binaries that form with Ap or Bp star companions will experience systemic angular-momentum losses due t…

astro-ph2005★ 54 cited

Models of Ultraluminous X-Ray Sources with Intermediate-Mass Black Holes

N. Madhusudhan, S. Justham, L. Nelson +4

We have computed models for ultraluminous X-ray sources ("ULXs") consisting of a black-hole accretor of intermediate mass ("IMBH"; e.g., ~1000 Msun) and a captured donor star. For…

astro-ph2005★ 13 cited

An Infrared Imaging Survey of the Faint Chandra Sources near the Galactic Centre

R. M. Bandyopadhyay, J. C. A. Miller-Jones, K. M. Blundell +6

We present near-IR imaging of a sample of the faint, hard X-ray sources discovered in the 2001 Chandra ACIS-I survey towards the Galactic Centre (GC) (Wang et al. 2002). These ~800…

astro-ph2005★ 54 cited

The spin period - eccentricity relation of double neutron stars: evidence for weak supernova kicks?

J D M Dewi, Ph Podsiadlowski, O R Pols

Double neutron stars (DNSs), binary systems consisting of a radio pulsar and a generally undetected second neutron star (NS), have proven to be excellent laboratories for testing t…

astro-ph2005★ 125 cited

The Double Pulsar J0737--3039: Testing the Neutron Star Equation of State

Ph. Podsiadlowski, J. D. M. Dewi, P. Lesaffre +3

The double pulsar J0737--3039 has become an important astrophysical laboratory for testing fundamental physics. Here we demonstrate that the low measured mass of Pulsar B can be us…

astro-ph2005★ 64 cited

Relativistic Binary Pulsars with Black-Hole Companions

Eric Pfahl, Philipp Podsiadlowski, Saul Rappaport

Binaries containing a stellar-mass black hole and a recycled radio pulsar have so far eluded detection. We present a focused investigation of the formation and evolution of these s…

astro-ph2005★ 181 cited

High-Velocity Features: a ubiquitous property of Type Ia SNe

P. A. Mazzali, S. Benetti, G. Altavilla +26

Evidence of high-velocity features such as those seen in the near-maximum spectra of some Type Ia Supernovae (eg SN 2000cx) has been searched for in the available SNIa spectra obse…

astro-ph2005★ 40 cited

Anisotropic mass ejection in binary mergers

T. Morris, Ph. Podsiadlowski

We investigate the mass loss from a rotationally distorted envelope following the early, rapid in-spiral of a companion star inside a common envelope. For initially wide, massive b…

astro-ph2005

Exploring the Nature of Weak Chandra Sources near the Galactic Centre

R. M. Bandyopadhyay, J. C. A. Miller-Jones, K. M. Blundell +5

We present results from the first near-IR imaging of the weak X-ray sources discovered in the Chandra/ACIS-I survey (Wang et al. 2002) towards the Galactic Centre (GC). These ~800…