Skip to search formSkip to main contentSkip to account menu
Swings between rotation and accretion power in a binary millisecond pulsar
TLDR
Observations of accretion-powered, millisecond X-ray pulsations from a neutron star previously seen as a rotation- powered radio pulsar show the evolutionary link between accretion and rotation-powered millisecond pulsars, but also that some systems can swing between the two states on very short timescales.
View on Nature
A radio continuum study of the Magellanic Clouds - VII. Discrete radio sources in the Magellanic Clouds
We present a study of discrete radio sources in the Magellanic Clouds (MCs) using the latest large-scale radio surveys made with the Parkes radio telescope be- tween 1.4 and 8.55 GHz. These surveys…
View via Publisher
An Australia Telescope Compact Array 20-cm radio continuum study of the Large Magellanic Cloud
We present a mosaic image of the 1.4-GHz radio continuum emission from the Large Magellanic Cloud (LMC) observed with the Australia Telescope Compact Array (ATCA) and the Parkes Telescope. The mosaic…
View via Publisher
Science with the Cherenkov Telescope Array
The Cherenkov Telescope Array, CTA, will be the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond. The scientific potential of CTA is extremely broad:…
View PDF on arXiv
A multiresolution analysis of the radio-FIR correlation in the Large Magellanic Cloud
We investigate the local correlation between the 1.4-GHz radio continuum and 60-μm far-infrared (FIR) emission within the Large Magellanic Cloud (LMC) on spatial scales between 0.05 and 1.5 kpc. On…
View PDF on arXiv
SXP 1062, a young Be X-ray binary pulsar with long spin period - implications for the neutron star birth spin
Context. The Small Magellanic Cloud (SMC) is ideally suited to investigating the recent star formation history from X-ray source population studies. It harbours a large number of Be/X-ray binaries…
View PDF on arXiv
An ATCA radio-continuum study of the Small Magellanic Cloud — III. Supernova remnants and their environments
A total of 717 sources from the Australia Telescope Compact Array (ATCA) catalogue of the Small Magellanic Cloud (SMC) have been classified in Paper II (of this series) by Payne et al. Here, we…
View via Publisher
A ROSAT PSPC catalogue of X-ray sources in the SMC region ?
We present a catalogue of 517 discrete X-ray sources in a 66 eld covering the Small Magellanic Cloud (SMC). The catalogue was derived from the pointed ROSAT PSPC observations performed between…
View via Publisher
An ATCA radio-continuum study of the Small Magellanic Cloud – I. Source catalogues at 1.42, 2.37, 4.80 and 8.64 GHz
We have analysed radio-continuum mosaics of the Small Magellanic Cloud (SMC) obtained using both the Australia Telescope Compact Array (ATCA) and the Parkes telescope and present a new catalogue of…
View via Publisher
An ATCA radio‐continuum study of the Small Magellanic Cloud – V. Long‐slit optical spectroscopy of supernova remnants and confirmation of a new candidate supernova remnant
We present optical long-slit spectra and estimated line ratios for 11 of the 16 known radio supernova remnants (SNRs) in the Small Magellanic Cloud (SMC) using observations made with the 2.3-m…
View via Publisher
...
...
By clicking accept or continuing to use the site, you agree to the terms outlined in our Privacy Policy, Terms of Service, and Dataset License