Zobrazeno 1 - 10
of 96
pro vyhledávání: '"J. H. Swank"'
Autor:
C. G. Montgomery, J. H. Swank
The polarization of an X-ray beam that produces electrons with velocity components perpendicular to the beam generates an azimuthal distribution of the ejected electrons. We present methods for simulating and for analyzing the angular dependence of e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c2660a87d415da91b8dac7ea4a22a1fd
http://arxiv.org/abs/1501.02222
http://arxiv.org/abs/1501.02222
Autor:
J. H. Swank
Publikováno v:
Advances in Space Research. 38:2959-2963
The prime scientific objectives of the Rossi X-Ray Timing Explorer (RXTE) were the study of astrophysical compact objects: black holes (galactic and extragalactic), many types of neutron stars, and accreting white dwarfs. RXTE was successful in achie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a50b153a8cd623d74b7d4a63a8f319b9
https://doi.org/10.1016/j.asr.2006.07.009
https://doi.org/10.1016/j.asr.2006.07.009
Publikováno v:
The Astrophysical Journal. 616:463-468
XMM-Newton observed SAX J2103.5+4545 on January 6, 2003, while RXTE was monitoring the source. Using RXTE-PCA dataset between December 3, 2002 and January 29, 2003, the spin period and average spin-up rate during the XMM-Newton observations were foun
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3082e68d167ff514b80b88d5c114116f
https://doi.org/10.1086/424825
https://doi.org/10.1086/424825
Publikováno v:
The Astrophysical Journal. 578:L129-L132
Five years of Rossi X-ray Timing Explorer (RXTE) observations of the Galactic black-hole candidates 1E 1740.7-2942 and GRS 1758-258 show a periodic modulation with amplitude 3-4% in each source at 12.73 +/- 0.05 dy and 18.45 +/- 0.10 dy, respectively
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1b0695a08367623adb06661dadcc39ac
https://doi.org/10.1086/344701
https://doi.org/10.1086/344701
We present a timing analysis of X Persei (X Per) using observations made between 1998 and 2010 with the Proportional Counter Array (PCA) onboard the Rossi X-ray Timing Explorer (RXTE) and with the INTEGRAL Soft Gamma-Ray Imager (ISGRI). All pulse arr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b547152930a3315c1aeeef1e7c75ba31
https://aperta.ulakbim.gov.tr/record/62137
https://aperta.ulakbim.gov.tr/record/62137
Autor:
Michael F. Corcoran, J. H. Swank, Robert Petre, Roberto Viotti, Kris Davidson, Augusto Damineli, Randall Smith, Kazunori Ishibashi, Simon D. M. White, Leisa K. Townsley
Publikováno v:
The Astrophysical Journal. 562:1031-1037
Eta Car may be the most massive and luminous star in the Galaxy and is suspected to be a massive, colliding wind binary system. The CHANDRA X-ray observatory has obtained a calibrated, high-resolution X-ray spectrum of the star uncontaminated by the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1fd77920406db5b4609d91c44f13f967
https://doi.org/10.1086/323322
https://doi.org/10.1086/323322
Publikováno v:
The Astrophysical Journal. 545:420-428
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e8de987b8030f28ebe7651232c1b8a2a
https://doi.org/10.1086/317806
https://doi.org/10.1086/317806
Publikováno v:
Advances in Space Research. 25:383-386
The type I X-ray burster 1E1724-3045 located in the globular cluster Terzan 2 was observed by the Rossi X-ray Timing Explorer (RXTE) while it was in a Island state, displaying both intense flickering and a hard Comptonized spectrum. No statistically
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::34a332bc2c58486e33ad41cf2d626da1
https://doi.org/10.1016/s0273-1177(99)00763-2
https://doi.org/10.1016/s0273-1177(99)00763-2
Autor:
Stephen M. White, Stephen A. Drake, Michael F. Corcoran, Augusto Damineli, J. H. Swank, K. Ishibashi, Robert Petre, K. Davidson
Publikováno v:
The Astrophysical Journal. 524:983-987
Recent studies suggest that, the super-massive star eta Carinae may have a massive stellar companion (Damineli, Conti, and Lopes 1997), although the dense ejecta surrounding the star make this claim hard to test using conventional methods. Settling t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5c603a6d177b23f5fc96c41957b797e9
https://doi.org/10.1086/307859
https://doi.org/10.1086/307859
Autor:
D. R. MacDonald, S. E. Woosley, Keith Jahoda, Philip Blanco, Michael R. Pelling, Richard E. Rothschild, K. Nomoto, Richard E. Lingenfelter, G. E. Allen, J. C. Higdon, William A. Heindl, J. H. Swank, Duane Gruber, D. Marsden
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 69:68-73
Rossi X-ray Timing Explorer (RXTE) observations of the bright supernova remnant Cas A have revealed a hard power law component above 10 keV in addition to two thermal components inferred from ASCA measurements of the many line centroids from low-Z el
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0ad6230b0fa3ab69472d43938e571c7a
https://doi.org/10.1016/s0920-5632(98)00186-8
https://doi.org/10.1016/s0920-5632(98)00186-8