Zobrazeno 1 - 10
of 38
pro vyhledávání: '"C. R. Gwinn"'
Publikováno v:
The Strongest Magnetic Fields in the Universe ISBN: 9781493935499
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e91fc992178af820d0e8c17ed7687d4e
https://doi.org/10.1007/978-1-4939-3550-5_7
https://doi.org/10.1007/978-1-4939-3550-5_7
Autor:
C. R. Gwinn
Publikováno v:
Astronomical & Astrophysical Transactions. 26:525-533
Levy flights are similar to random walks, but are dominated by rare, large events rather than the accumulation of many steps. Levy flights are not subject to the Central Limit Theorem because the distribution of steps has no second moment; they conve
Publikováno v:
Space Science Reviews, vol 191, iss 1-4
Almost 50 years after radio pulsars were discovered in 1967, our understanding of these objects remains incomplete. On the one hand, within a few years it became clear that neutron star rotation gives rise to the extremely stable sequence of radio pu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3007da60b9b69ed253d5d0c56563211b
https://escholarship.org/uc/item/1tv744t5
https://escholarship.org/uc/item/1tv744t5
Autor:
C. R. Gwinn, M. C. Britton, J. E. Reynolds, D. L. Jauncey, E. A. King, P. M. McCulloch, J. E. J. Lovell, R. A. Preston
Publikováno v:
The Astrophysical Journal. 505:928-940
Autor:
C. R. Gwinn, M. J. Ojeda, M. C. Britton, J. E. Reynolds, D. L. Jauncey, E. A. King, P. M. McCulloch, J. E. J. Lovell, C. S. Flanagan, D. P. Smits, R. A. Preston, D. L. Jones
Publikováno v:
The Astrophysical Journal. 483:L53-L56
We use interstellar scattering of the Vela pulsar to determine the size of its emission region. From interferometric phase variations on short baselines, we find that radio-wave scattering broadens the source by 3.4+/-0.3 milliarcseconds along the ma
Publikováno v:
Infrared Astronomy with Arrays ISBN: 9789401044660
We discuss some theoretical and practical considerations relating to achieving spatial resolution higher than ~ λ/D, the nominal diffraction-limited resolution of a telescope of diameter D. Although the Nyquist criterion is often invoked as a justif
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::014940692f10ddcb98f0e9a995f00e46
https://doi.org/10.1007/978-94-011-1070-9_97
https://doi.org/10.1007/978-94-011-1070-9_97
Autor:
C. R. Gwinn
Publikováno v:
Astrophysical Masers ISBN: 9783540563433
Observations of 105 H2O maser features in W49N indicate that high-velocity features lie at the periphery of the maser outflow. Model fits indicate that the high-velocity features lie at either end of a bipolar outflow. A high-velocity stellar wind ma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::928677ab7d68edc71b38697709adf824
https://doi.org/10.1007/3-540-56343-1_252
https://doi.org/10.1007/3-540-56343-1_252
Publikováno v:
Experimental Astronomy. 3:153-154
Publikováno v:
The Astrophysical Journal. 447:391
Autor:
C. R. Gwinn
Publikováno v:
The Astrophysical Journal. 431:L123