Results 31 to 40 of about 769,577 (231)
The LOFAR pilot surveys for pulsars and fast radio transients [PDF]
, 2014 We have conducted two pilot surveys for radio pulsars and fasttransients with the Low-Frequency Array (LOFAR) around 140 MHz and herereport on the first low-frequency fast-radio burst limit and thediscovery of two new pulsars. The first survey, the LOFAR Röttgering, H., Wucknitz, O, Weltevrede, Patrick, McFadden, R., Garrett, MA, M. Brüggen, Wijnholds, S., van Amesfoort, A. S., Hassall, T., Brüggen, M, Griessmeier, Jean-Mathias, Kuniyoshi, M, Orru, E, Karastergiou, A., Corstanje, A., Garrett, M., Hessels, Jason W T, McKay-Bukowski, D., Thoudam, S, Tasse, C, Hassall, T E, Sluman, J, Zensus, A, Kramer, M, van Weeren, R., C. Sobey, Zagkouris, K, Broderick, J, Kuper, G, Brüggen, M., Hassall, TE, Bilous, A, Rowlinson, A, Pilia, M., Sobey, Charlotte, van der Horst, A., T. E. Hassall, Fender, R, Hessels, Jason W. T., Ciardi, B., Noutsos, A, Falcke, H, Jason W. T. Hessels, Vladislav I. Kondratiev, M. J. Bentum, Röttgering, H, Anderson, J., Gajjar, V., Keane, EF, M. E. Bell, Noutsos, A., Schwarz, D, S. Cooper, Stappers, B.W., Grießmeier, J-M, Griessmeier, J-M., Paas, H., Butcher, H., E. Juette, Sobey, C., van Weeren, R. J., Karastergiou, A, Verbiest, J, van Weeren, RJ, A. van der Horst, Weltevrede, P, Bell, M. E., Hoeft, M., R. P. Breton, Verbiest, J., Mann, G., Keane, E., Renting, A., J. Broderick, Butcher, HR, Hamaker, J., Kuper, G., H. Röttgering, G. Mann, Hassall, T.E., Hassall, T. E., K. Zagkouris, Garrett, Michael; id_orcid, Toribio, C, Grießmeier, J., Tagger, M., Thoudam, S., Grießmeier, J.-M., Cooper, S., Osłowski, S., I. M. Avruch, W. Reich, Polatidis, A G, Eislöffel, J., R. McFadden, Juette, E., Munk, H, Griessmeier, J.M., A. Bilous, Kondratiev, VI, C. Schrijvers, Kondratiev, Vladislav I., A. M. M. Scaife, Veen, S., Garrett, M. A., Amesfoort, A., Schrijvers, C., Thijs Coenen, Bell, M E, Deller, A., Fallows, R A, R. Fender, Zarka, P., Bell, ME, Schwarz, Dominik ; https://orcid.org/, Bonafede, A, Kondratiev, V., Pilia, M, Sobey, C, Heald, G., Tagger, Michel, Garrett, M.A., van Leeuwen, J., P. Zarka, Smirnov, O., Keane, E. F., van Weeren, R J, Bell, M., Breton, Rene P; id_orcid, Oslowski, S., J. Anderson, C. Ferrari, Avruch, IM, et al., C. Law, J.-M. Grießmeier, Alexov, A, Scaife, A M M; id_orcid, Serylak, M, E. Orru, McKean, J P, Thoudam, Satyendra,, O. Smirnov, Scaife, AMM, Breitling, F., Hamaker, J P, M. Hoeft, Coenen, Thijs, Butcher, H. R., Avruch, I., G. Bernardi, A. Corstanje, Hessels, J., Kramer, M., Brueggen, M, R. J. van Weeren, Scaife, A., S. Duscha, Gunst, A. W., Best, P, Corstanje, A, van Amesfoort, A S, Zagkouris, K., Bernardi, G., S. Osłowski, Broderick, J., de Geus, E., McKean, J., McKean, J. P., C. Tasse, Swinbank, J., et al, Vocks, C., A. W. Gunst, Vocks, C, Oslowski, Stefan, Schwarz, D., Bernardi, G, A. Karastergiou, Breitling, F, Breton, R.P., D. McKay-Bukowski, Gasperin, F., Tasse, C., Stappers, Benjamin W; id_orcid, A. G. Polatidis, Cooper, S, ter Veen, S, Gunst, A., F. Breitling, et al., [Unknown], A. Noutsos, Deller, A, Sluman, J., McKean, JP, Joeri van Leeuwen, Brueggen, M., Veen, S. ter, Oslowski, S, V. Gajjar, M. Serylak, Gajjar, V, R. Vermeulen, Kuniyoshi, M., E. F. Keane, M. Kramer, M. Pilia, Gunst, A W, van der Horst, A, Y. Tang, Asgekar, A., Fallows, R., van Leeuwen, J, Bilous, A., Scaife, A. M. M., Juette, E, Gunst, AW, Stappers, Ben W., Fallows, RA, Bentum, M J, Hoeft, M, Ferrari, C., J. P. Hamaker, Ben W. Stappers, Keane, E F, Geus, E., Toribio, C., Coenen, T., Kondratiev, Vladislav I, M. A. Garrett, Eisloeffel, J., McKay-Bukowski, D, Kondratiev, V.I., Wijnholds, S, Stappers, B., G. Heald, Horst, A., Asgekar, A, P. Best, H. Munk, Mann, G, Hessels, JWT, van Amesfoort, AS, Coenen, T.J., B. Ciardi, Bentum, M. J., J. P. McKean, Zensus, A., S. Thoudam, Stappers, BW, Ciardi, B, Hessels, J. W. T., Anderson, J, Bentum, Marinus Jan, Verbiest, Joris ; https://orcid.org/, A. Rowlinson, ter Veen, S., M. Pandey-Pommier, Paas, H, Kondratiev, V. I., Polatidis, A. G., Hessels, J.W.T., G. Kuper, Eislöffel, J, Falcke, H., Leeuwen, J., Bentum, M., Rowlinson, A., S. Wijnholds, Pandey-Pommier, M, Polatidis, A., Eisloeffel, J, Hamaker, JP, Tagger, M, Orru, E., Serylak, M., Smirnov, O, A. Zensus, Polatidis, AG, Röttgering, H.J.A., Stappers, B. W., H. Falcke, W. Frieswijk, A. Renting, Hamaker, J. P., C. Vocks, Heald, G, A. Deller, M. Tagger, Bonafede, A., Schrijvers, C, J. Swinbank, Fender, R., S. ter Veen, D. Schwarz, E. de Geus, Law, C, R. A. Fallows, O. Wucknitz, A. Alexov, de Geus, E, F. de Gasperin, J. Eislöffel, A. Asgekar, Law, C., Renting, A, Fallows, R. A., Best, P., Frieswijk, W., Van Amesfoort, A., Ferrari, C, Wucknitz, O., Osłowski, S, J. Verbiest, de Gasperin, F, H. R. Butcher, Frieswijk, W, Tang, Y, Breton, R., Swinbank, J, P. Weltevrede, H. Paas, Coenen, T, Vermeulen, R., Butcher, H R, de Gasperin, F., Os\lowski, S., van Leeuwen, Joeri, Weltevrede, P., Alexov, A., Zarka, P, Grießmeier, J. -M., Breton, R. P., Reich, W., Grießmeier, J. -M, McFadden, R, J. Sluman, Avruch, I. M., Bentum, MJ, Reich, W, A. S. van Amesfoort, Avruch, I M, Breton, RP, Pandey-Pommier, M., Fallows, R.A., Duscha, S., C. Toribio, M. Kuniyoshi, Tang, Y., Duscha, S, A. Bonafede, Munk, H., Vermeulen, R +352 morecore +3 more sourcesAre radio pulsars strange stars ? [PDF]
Astronomy & Astrophysics, 2001 A remarkably precise observational relation for pulse core component widths of radio pulsars is used to derive stringent limits on pulsar radii, strongly indicating that pulsars are strange stars rather than neutron stars. This is achieved by inclusion of general relativistic effects due to the pulsar mass on the size of the emission region needed to ...Kapoor, R. C., Shukre, C. S.openaire +2 more sourcesMagnetic fields of radio pulsars [PDF]
Astronomy Reports, 2017 We used the magneto-dipole radiation mechanism for the braking of radio pulsars to calculate the new values of magnetic inductions at the surfaces of neutron stars. For this aim we estimated the angles ? between the rotation axis and the magnetic moment of the neutron star for 376 radio pulsars using three different methods. It was shown that there was Nikitina, E. B., Malov, I. F.openaire +2 more sourcesGravitoastronomy with neutron stars [PDF]
, 2004 Recent advances in gravitational wave detectors mean that we can start to make astrophysically important
statements about the physics of neutron stars based on observed upper limits to their gravitational luminosity.Woan, G., Graham Woancore +1 more sourceThe specifics of pulsar radio emission
Open Astronomy, 2022 A characteristic property of pulsars is pulsed periodic radio emission, which has a high stability of periods. Despite the high stability of the emission periods of pulsars, monitoring the time of arrival of pulses (timing) shows the presence of ...Losovsky Boris Ya.doaj +1 more source
