Zobrazeno 1 - 10
of 103
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
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
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
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
Publikováno v:
The Astrophysical Journal. 547:1034-1039
We solve the RXTE X-ray lightcurve of the extremely luminous and massive star eta Carinae with a colliding wind emission model to refine the ground-based orbital elements. The sharp decline to X-ray minimum at the end of 1997 fixes the date of the la
Publikováno v:
The Astrophysical Journal. 545:420-428
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
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