Zobrazeno 1 - 10
of 459
pro vyhledávání: '"Pelling M"'
Publikováno v:
Diabetes, Metabolic Syndrome and Obesity, Vol Volume 17, Pp 3111-3130 (2024)
Lina Shibib,1 Mo Al-Qaisi,1 Nicola Guess,2 Alexander D Miras,3 Steve E Greenwald,4 Marc Pelling,1 Ahmed Ahmed1 1Department of Surgery and Cancer, Imperial College London, London, UK; 2Nuffield Department of Primary Care Health Sciences, Oxford Univer
Externí odkaz:
https://doaj.org/article/45552ab0aeaf4e4db8e84cec0b559844
Publikováno v:
Vascular Health and Risk Management, Vol Volume 18, Pp 417-443 (2022)
Lina Shibib,1 Mo Al-Qaisi,1 Ahmed Ahmed,1 Alexander D Miras,2 David Nott,1 Marc Pelling,1 Stephen E Greenwald,3 Nicola Guess4 1Department of Surgery and Cancer, Imperial College London, London, UK; 2Department of Metabolism, Digestion and Reproductio
Externí odkaz:
https://doaj.org/article/c741f911cccc41649be86269c281681c
Autor:
D'Amico, F., Heindl, W. A., Rothschild, R. E., Peterson, L. E., Gruber, D. E., Pelling, M., Tomsick, J. A.
Using the HEXTE experiment on-board the RXTE satellite, we performed a search for hard X-ray tails in Sco X-1 spectra. We found strong evidence for the presence of such a non-thermal component on several occasions. Using the PCA/RXTE we were able to
Externí odkaz:
http://arxiv.org/abs/astro-ph/0101396
Autor:
Heindl, W. A., Coburn, W., Gruber, D. E., Pelling, M., Rothschild, R. E., Kretschmar, P., Kreykenbohm, I., Wilms, J., Pottschmidt, K., Staubert, R.
In this paper, we summarize the RXTE measurements of cyclotron resonance scattering features in 8 accreting pulsars. The wide bandpass and modest resolution of the RXTE instruments make them ideal for measuring these generally broad features. In part
Externí odkaz:
http://arxiv.org/abs/astro-ph/0004300
Autor:
Heindl, W. A., Coburn, W., Gruber, D. E., Pelling, M., Rothschild, R. E., Wilms, J., Pottschmidt, K., Staubert, R.
We report phase resolved spectroscopy of the transient accreting pulsar, 4U0115+63. For the first time, more than two cylotron resonance scattering features are detected in the spectrum of an X-ray pulsar. The shape of the fundamental line appears to
Externí odkaz:
http://arxiv.org/abs/astro-ph/0004297
Autor:
Coburn, W., Heindl, W. A., Wilms, J., Gruber, D. E., Staubert, R., Rothschild, R. E., Postnov, K. A., Shakura, N., Risse, P., Kreykenbohm, I., Pelling, M. R.
A failed main-on in the 35d cycle of Her X-1 was observed with the Rossi X-Ray Timing Explorer (RXTE) on 1999 April 26. Exceptions to the normal 35d cycle have been seen only twice before; in 1983 and again 1993. We present timing and spectral result
Externí odkaz:
http://arxiv.org/abs/astro-ph/9911533
Autor:
Heindl, W. A., Coburn, W., Gruber, D. E., Pelling, M. R., Rothschild, R. E., Wilms, J., Pottschmidt, K., Staubert, R.
We have discovered a third harmonic cyclotron resonance scattering feature (CRSF) in observations of the recent outburst of 4U 0115+63 with the Rossi X-ray Timing Explorer (RXTE). The spectrum in a narrow pulse phase range shows CRSFs at 12.40+0.65/-
Externí odkaz:
http://arxiv.org/abs/astro-ph/9904222
We report on the discovery of a new pulsating X-ray source during Rossi X-ray Timing Explorer observations of a low galactic latitude field centered at RA (J2000) = 19 hr 05 m 43 s and Dec (J2000) = +08 deg 58 arcmin 48 arcsec. Significant pulsations
Externí odkaz:
http://arxiv.org/abs/astro-ph/9805354
Autor:
Rothschild, R. E., Blanco, P. R., Gruber, D. E., Heindl, W. A., MacDonald, D. R., Marsden, D. C., Pelling, M. R., Wayne, L. R., Hink, P. L.
The High Energy X-ray Timing Experiment (HEXTE) is one of three scientific instruments aboard the Rossi X-ray Timing Explorer (RXTE), which was launched on December 30, 1995. RXTE performs timing and spectral studies of bright x-ray sources to determ
Externí odkaz:
http://arxiv.org/abs/astro-ph/9710328
Autor:
Marsden, D., Blanco, P. R., Gruber, D. E., Heindl, W. A., Pelling, M. R., Peterson, L. E., Rothschild, R. E., Rots, A. H., Jahoda, K., Macomb, D. J.
We present the results of observations of the PSR B1509$-$58/MSH 15$-$52 system in X-rays ($2-250$ keV) by the Rossi X-ray Timing Explorer. The spectra of the peak of the pulsed component (radio phase $0.17-0.53$) is fit by a power law of photon inde
Externí odkaz:
http://arxiv.org/abs/astro-ph/9710114