https://catalogue-scientifique.canada.ca/record=1301949~S6*frc
Academic Press, 1985, ISBN : 0121820106
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De : Réseau des bibliothèques scientifiques fédérales
https://catalogue-scientifique.canada.ca/record=1301949~S6*frc
https://catalogue-scientifique.canada.ca/record=1448449~S6*frc
https://catalogue-scientifique.canada.ca/record=1131371~S6*frc
https://publications-cnrc.canada.ca/fra/voir/objet/?id=d1052877-1397-4177-a24e-3598fb1a190b
We present results of a search for late-time radio emission and fast radio bursts (FRBs) from a sample of type-I superluminous supernovae (SLSNe-I). We used...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=5f64da42-be8d-4416-97f8-c7a66d274820
Aims. This work provides an update to existing reconstructions of the Galactic Faraday rotation sky by processing almost all Faraday rotation data sets...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=b9a66e95-1c9c-4b98-ae84-38b9213c9e7f
Radio interferometers have the ability to precisely localize and better characterize the properties of sources. This ability is having a powerful impact on the...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=ba9dde5d-cdb1-4948-80a2-7d3a6223ce20
Context. Molecular filaments and hubs have received special attention recently thanks to new studies showing their key role in star formation. While the...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=c36a0613-5d27-429c-a1e1-75329bf9706c
Fast radio bursts (FRBs) are brief, bright, extragalactic radio flashes (1,2). Their physical origin remains unknown, but dozens of possible models have been...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=9fad8d1a-27a9-4ce8-9e77-69caf8d4519c
We undertook coordinated campaigns with the Green Bank, Effelsberg, and Arecibo radio telescopes during Chandra X-ray Observatory and XMM-Newton observations...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=035eabc9-1ab3-4426-9977-968d925377a2
FRB 121102 is the only known repeating fast radio burst source. Here we analyze a wide-frequency-range (1–8 GHz) sample of high signal-to-noise, coherently...
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