activity
19972004
most citedPSR B1951+32: A Bow Shock-Confined X-ray Nebula, a Synchrotron Knot and an Optical Counterpart Candidate

24 citations · 56 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph2004★ 24 cited

PSR B1951+32: A Bow Shock-Confined X-ray Nebula, a Synchrotron Knot and an Optical Counterpart Candidate

D. -S. Moon, J. -J. Lee, S. S. Eikenberry +7

The radio pulsar B1951+32 and the supernova remnant CTB 80 provide a rich laboratory for the study of neutron stars and supernova remnants. Here, we present ground-based optical an…

astro-ph2002★ 10 cited

Understanding the LMXB X2127+119 in M15

Zach Ioannou, L. van Zyl, T. Naylor +4

We present HST UV observations of the high-inclination low mass X-ray binary AC211 (X2127+119), which is located in the globular cluster M15 (NGC 7078). We have discovered a CIV P…

astro-ph2002

SS433: the second Wolf-Rayet X-ray binary ?

Yael Fuchs, Lydie Koch-Miramond, Peter Abraham

We present mid-infrared spectrophotometric observations of SS433 with ISOPHOT. The HeI+HeII lines in both spectra of SS433 and of the Wolf-Rayet star WR147, a wind-colliding WN8+BO…

astro-ph2002★ 22 cited

A 2.4 - 12 microns spectrophotometric study with ISO of Cygnus X-3 in quiescence

Lydie Koch-Miramond, P'eter 'Abrah'am, Ya"el Fuchs +2

We present mid-infrared spectrophotometric results obtained with the ISO on the peculiar X-ray binary Cygnus X-3 in quiescence, at orbital phases 0.83 to 1.04. The 2.4-12 microns c…

astro-ph1997

Astrometry of the globular cluster 47 Tuc and possible optical identification of X-ray sources

M. Geffert, M. Auriere, L. Koch-Miramond

Positions of stars of 47 Tuc have been derived by the use of photographic plates and CCD frames (ESO La Silla) and data from the Hubble Space Telescope (HST). The positions have be…