Zobrazeno 1 - 10
of 57
pro vyhledávání: '"Blundell, KM"'
We examine limits to the energy to which cosmic rays can be accelerated by relativistic shocks, showing that acceleration of light ions as high as 100 EeV is unlikely. The implication of our estimates is that if ultra-high energy cosmic rays are acce
Externí odkaz:
http://arxiv.org/abs/1709.07793
Autor:
Broderick, JW, Fender, RP, Miller-Jones, JCA, Trushkin, SA, Stewart, AJ, Anderson, GE, Staley, TD, Blundell, KM, Pietka, M, Markoff, S, Rowlinson, A, Swinbank, JD, van der Horst, AJ, Bell, ME, Breton, RP, Carbone, D, Corbel, S, Eislöffel, J, Falcke, H, Grießmeier, JM, Hessels, JWT, Kondratiev, VI, Law, CJ, Molenaar, GJ, Serylak, M, Stappers, BW, van Leeuwen, J, Wijers, RAMJ, Wijnands, R, Wise, MW, Zarka, P
© 2017 The Author(s). We present Low-Frequency Array (LOFAR) high-band data over the frequency range 115-189 MHz for the X-ray binary SS 433, obtained in an observing campaign from 2013 February to 2014 May. Our results include a deep, wide-field ma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______363::294be9a7730d8770142d15a78e43d569
https://hdl.handle.net/10453/125930
https://hdl.handle.net/10453/125930
Multifrequency VLA and OVRO observations of the radio outburst of Cygnus X-3 in September 2001 are presented, illustrating the evolution of the spectrum of the source over a period of six days. An estimate of the magnetic field in the emitting region
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2dc0d999d30462e8b25e8eb457c3cd0f
https://ora.ox.ac.uk/objects/uuid:787e57c9-4db1-4792-b83c-3208bb535abb
https://ora.ox.ac.uk/objects/uuid:787e57c9-4db1-4792-b83c-3208bb535abb
Chandra observations of 3C432, 3C191 and B2 0902+34 are presented as part of an ongoing search for inverse-Compton scattering of the cosmic microwave background (CMB) from high redshift radio sources (Schwartz, 2000). The energy density of the CMB in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::7d93bcb6fe80fc76a96f1e0066596628
https://ora.ox.ac.uk/objects/uuid:ecf0ed57-9c09-4338-9c0b-1bf7ae68a4e2
https://ora.ox.ac.uk/objects/uuid:ecf0ed57-9c09-4338-9c0b-1bf7ae68a4e2
Autor:
Sebastian Perez, M, Blundell, KM
A succession of near-IR spectroscopic observations, taken nightly throughout an entire cycle of SS 433's orbit with UKIRT, reveal (i) the persistent signature of SS 433's accretion disc, having a rotation speed of ∼ 500 kms-1and (ii) confirms the p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::636b5a89b7e52e384ab20f10acf073b6
https://ora.ox.ac.uk/objects/uuid:f53ce3f7-6886-4f00-bd22-1969ae46d0e8
https://ora.ox.ac.uk/objects/uuid:f53ce3f7-6886-4f00-bd22-1969ae46d0e8
[ABRIDGED] The distance to the relativistic jet source SS433 and the related supernova remnant W50 is re-examined using new observations of HI in absorption from the VLA, HI in emission from the GBT, and 12CO emission from the FCRAO. The new measurem
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=arXiv_dedup_::e88b3609001baa343f1a6258ed097e79
https://ora.ox.ac.uk/objects/uuid:0ed550f0-d155-48b0-beff-794a5c38426e
https://ora.ox.ac.uk/objects/uuid:0ed550f0-d155-48b0-beff-794a5c38426e
Using a new radio sample, 6C* designed to find radio galaxies at z > 4 along with the complete 3CRR and 6CE sample we extend the radio galaxy K - z relation to z - 4.5. The 6C* K - z data significantly improve delineation of the K - z relation for ra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::cf0cd5e3e5e12cccae1d244108482630
https://ora.ox.ac.uk/objects/uuid:139df9c3-37b9-4fc1-a787-5acb7a7b8cb5
https://ora.ox.ac.uk/objects/uuid:139df9c3-37b9-4fc1-a787-5acb7a7b8cb5
We present new Giant Metre-wave Radio Telescope (GMRT) observations of Hubble Deep Field (HDF)130, an inverse-Compton (IC) ghost of a giant radio source that is no longer being powered by jets. We compare the properties of HDF130 with the new and imp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::a57d1df4b45e6a857bd10aba74baa4c7
https://doi.org/10.1111/j.1365-2966.2011.19374.x
https://doi.org/10.1111/j.1365-2966.2011.19374.x
Autor:
Cruz, MJ, Jarvis, MJ, Blundell, KM, Rawlings, S, Croft, S, Klöckner, H-R, McLure, RJ, Simpson, C, Targett, TA, Willott, CJ, Kloeckner, HR
Publikováno v:
Mon.Not.Roy.Astron.Soc.373:1531-1562,2006. 373(4)
We present basic observational data on the 6C** sample. This is a new sample of radio sources drawn from the 151 MHz 6C survey, which was filtered with radio criteria chosen to optimize the chances of finding radio galaxies at z > 4. The filtering cr