180 citations
- University of ManchesterGB36 papers
- Netherlands Institute for Radio AstronomyNL7 papers
- California Institute of TechnologyUS6 papers
- Max Planck Institute for Radio AstronomyDE6 papers
- Joint Institute for VLBI ERICNL5 papers
- Université Paris CitéFR5 papers
- University of CambridgeGB5 papers
- Cornell UniversityUS4 papers
- University of British ColumbiaCA4 papers
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- Centre National de la Recherche ScientifiqueFR3 papers
- Consejo Superior de Investigaciones CientíficasES3 papers
13 papers · 1 filter
Simultaneous multi-wavelength observations of microquasars (the MINE collaboration)
Yael Fuchs, J. Rodriguez, I. F. Mirabel +9
We present the international collaboration MINE (Multi-lambda INTEGRAL NEtwork) aimed at conducting multi-wavelength observations of microquasars simultaneously with the INTEGRAL s…
New Planetary Nebulae in the Northern Galactic Plane
Panayotis Boumis, Myfanwy Bryce
We present deep Halpha+[N II] CCD images of selected new Planetary Nebulae (PNe) discovered through an [O III] 5007 A emission line survey in the Galactic Bulge region with l > 0 d…
Searching for sub-millisecond pulsars from highly polarized radio sources
J. L. Han, R. N. Manchester, A. G. Lyne +1
Pulsars are among the most highly polarized sources in the universe. The NVSS has catalogued 2 million radio sources with linear polarization measurements, from which we have selec…
Observational manifestations of young neutron stars: Spin-powered pulsars
Michael Kramer
The largest number of known young neutron stars are observed as spin-powered pulsars. While the majority of those are detected at radio frequencies, an increasing number can be stu…
Giant pulses in Millisecond Pulsars
B. C. Joshi, M. Kramer, A. G. Lyne +2
Giant pulses (GPs), occasional individual pulses with an intensity 100 times the average intensity, have been detected in four pulsars todate. Their origin is not well understood,…
The Most Detailed Picture Yet of an Embedded High-mass YSO
L. J. Greenhill, M. J. Reid, C. J. Chandler +2
High-mass star formation is not well understood chiefly because examples are deeply embedded, relatively distant, and crowded with sources of emission. Using VLA and VLBA observati…