Zobrazeno 1 - 10
of 117
pro vyhledávání: '"Wijers RAMJ"'
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
Autor:
Arias, Maria, Vink, J, De Gasperin, F, Salas, P, Oonk, JBR, Van Weeren, RJ, Van Amesfoort, AS, Anderson, J, Beck, R, Bell, ME, Bentum, MJ, Best, P, Blaauw, R, Breitling, F, Broderick, JW, Brouw, WN, Bruggen, M, Butcher, HR, Ciardi, B, De Geus, E, Deller, A, Van Dijk, PCG, Duscha, S, Eisloffel, J, Garrett, MA, Grie?meier, JM, Gunst, AW, Van Haarlem, MP, Heald, G, Hessels, J, Horandel, J, Holties, HA, Van Der Horst, AJ, Iacobelli, M, Juette, E, Krankowski, A, Van Leeuwen, J, Mann, G, McKay, Derek, McKean, JP, Mulder, H, Nelles, A, Orru, E, Paas, H, Pandey-Pommier, M, Pandey, VN, Pekal, R, Pizzo, R, Polatidis, AG, Reich, W, Rottgering, HJA, Rothkaehl, H, Schwarz, DJ, Smirnov, O, Soida, M, Steinmetz, M, Tagger, M, Thoudam, S, Toribio, MC, Vocks, C, Van Der Wiel, MHD, Wijers, RAMJ, Wucknitz, O, Zarka, P, Zucca, Philippe M.
Publikováno v:
Arias, M., Vink, J., de Gasperin, F., Salas, P., Oonk, J.B.R, van Weeren, R.J. ... Zucca, P. (2018). Low-frequency radio absorption in Cassiopeia A. Astronomy & Astrophysics, 612, A110.
Externí odkaz:
https://hdl.handle.net/10037/15168
Autor:
Buitink, S, Corstanje, A, Falcke, H, Hörandel, JR, Huege, T, Nelles, A, Rachen, JP, Rossetto, L, Schellart, P, Scholten, O, Ter Veen, S, Thoudam, S, Trinh, TNG, Anderson, J, Asgekar, A, Avruch, IM, Bell, ME, Bentum, MJ, Bernardi, G, Best, P, Bonafede, A, Breitling, F, Broderick, JW, Brouw, WN, Brüggen, M, Butcher, HR, Carbone, D, Ciardi, B, Conway, JE, De Gasperin, F, De Geus, E, Deller, A, Dettmar, RJ, Van Diepen, G, Duscha, S, Eislöffel, J, Engels, D, Enriquez, JE, Fallows, RA, Fender, R, Ferrari, C, Frieswijk, W, Garrett, MA, Grießmeier, JM, Gunst, AW, Van Haarlem, MP, Hassall, TE, Heald, G, Hessels, JWT, Hoeft, M, Horneffer, A, Iacobelli, M, Intema, H, Juette, E, Karastergiou, A, Kondratiev, VI, Kramer, M, Kuniyoshi, M, Kuper, G, Van Leeuwen, J, Loose, GM, Maat, P, Mann, G, Markoff, S, McFadden, R, McKay-Bukowski, D, McKean, JP, Mevius, M, Mulcahy, DD, Munk, H, Norden, MJ, Orru, E, Paas, H, Pandey-Pommier, M, Pandey, VN, Pietka, M, Pizzo, R, Polatidis, AG, Reich, W, Röttgering, HJA, Scaife, AMM, Schwarz, DJ, Serylak, M, Sluman, J, Smirnov, O, Stappers, BW, Steinmetz, M, Stewart, A, Swinbank, J, Tagger, M, Tang, Y, Tasse, C, Toribio, MC, Vermeulen, R, Vocks, C, Vogt, C, Van Weeren, RJ, Wijers, RAMJ, Wijnholds, SJ, Wise, MW
© 2016 Macmillan Publishers Limited. All rights reserved. Cosmic rays are the highest-energy particles found in nature. Measurements of the mass composition of cosmic rays with energies of 1017-1018 electronvolts are essential to understanding wheth
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______363::9d6e0fc1f331862f51f56bccc73544cd
https://hdl.handle.net/10453/113562
https://hdl.handle.net/10453/113562
Publikováno v:
van Eerten, H J, Meliani, Z, Wijers, R A M J & Keppens, R 2011, ' Jet simulations and gamma-ray burst afterglow jet breaks ', Monthly Notices of the Royal Astronomical Society, vol. 410, no. 3, pp. 2016-2024 . https://doi.org/10.1111/j.1365-2966.2010.17582.x
Monthly Notices of the Royal Astronomical Society, 410, 2016-2024
Monthly Notices of the Royal Astronomical Society, 410(3), 2016-2024. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 410, 2016-2024
Monthly Notices of the Royal Astronomical Society, 410(3), 2016-2024. Oxford University Press
The conventional derivation of the gamma-ray burst afterglow jet break time uses only the blast wave fluid Lorentz factor and therefore leads to an achromatic break. We show that in general gamma-ray burst afterglow jet breaks are chromatic across th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::68bb126c8d36174b6bf9b944d70b1033
https://doi.org/10.1111/j.1365-2966.2010.17582.x
https://doi.org/10.1111/j.1365-2966.2010.17582.x
Autor:
Galama, TJ, Briggs, MS, Wijers, RAMJ, Rol, E, Band, D, van Paradijs, J, Kouveliotou, C, Preece, RD, Smith, IA, Tilanus, RPJ, de Bruyn, AG, Strom, RG, Pooley, G, Castro-Tirado, AJ, Tanvir, N, Robinson, C, Hurley, K, Heise, J, Telting, J, Rutten, RGM, Packham, C, Swaters, R, Fassia, A, Green, SF, Foster, MJ, Sagar, R, Pandey, AK, Nilakshi, [No Value], Yadav, RKS, Ofek, EO, Leibowitz, E, Ibbetson, P, Rhoads, J, Falco, E, Petry, C, Impey, C, Geballe, TR, Bhattacharya, D
Publikováno v:
Nature, 398(6726), 394-399. Nature Publishing Group
Gamma-ray bursts (GRBs) are thought to arise when an extremely relativistic outflow of particles from a massive explosion (the nature of which is still unclear) Interacts with material surrounding the site of the explosion. observations of the evolvi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::a771b44e6003a5ee0189e8296c372d10
https://research.rug.nl/en/publications/552fcbe1-56a3-4c94-939e-f0a82401f376
https://research.rug.nl/en/publications/552fcbe1-56a3-4c94-939e-f0a82401f376
Autor:
Galama, TJ, Wijers, RAMJ, Groot, PJ, Strom, RG, De Bruyn, AG, Kouveliotou, C, Robinson, CR, van Paradus, J
Publikováno v:
Astrophysical Journal, 500(2), L101-L104. IOP PUBLISHING LTD
We report on Westerbork 1.4 GHz radio observations of the radio counterpart to gamma-ray burst GRB 970508, between 0.80 and 138 days after this event. The 1.4 GHz light curve shows a transition from optically thick to thin emission between 39 and 54
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::0736f7158501a01764b94672b942fdb5
https://research.rug.nl/en/publications/61883b91-df28-4151-b938-8e7a7c96c325
https://research.rug.nl/en/publications/61883b91-df28-4151-b938-8e7a7c96c325
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