Zobrazeno 1 - 10
of 298
pro vyhledávání: '"Barragán L"'
Autor:
del Baño-Barragán, L., Martínez-García, Á., Garríguez-Pérez, D., Mora-Fernández, J., García-Coiradas, J., Valle-Cruz, J.A., Marco, F.
Publikováno v:
In Revista Espanola de Cirugia Ortopedica y Traumatologia June 2024
Akademický článek
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Autor:
Martinez-Medina, Gloria A., Chávez-González, Mónica L., Verma, Deepak Kumar, Prado-Barragán, L. Arely, Martínez-Hernández, Jose L., Flores-Gallegos, Adriana C., Thakur, Mamta, Srivastav, Prem Prakash, Aguilar, Cristóbal N.
Publikováno v:
In Journal of Functional Foods February 2021 77
Autor:
Caballero, I., Pottschmidt, K., Marcu, D. M., Barragan, L., Ferrigno, C., Klochkov, D., Heras, J. A. Zurita, Suchy, S., Wilms, J., Kretschmar, P., Santangelo, A., Kreykenbohm, I., Fürst, F., Rothschild, R., Staubert, R., Finger, M. H., Camero-Arranz, A., Makishima, K., Enoto, T., Iwakiri, W., Terada, Y.
The Be/X-ray binary A 0535+26 showed a normal (type I) outburst in August 2009. It is the fourth in a series of normal outbursts associated with the periastron, but is unusual by presenting a double-peaked light curve. The two peaks reached a flux of
Externí odkaz:
http://arxiv.org/abs/1301.4856
Autor:
Pottschmidt, K., Suchy, S., Rivers, E., Rothschild, R. E., Marcu, D. M., Barragán, L., Kühnel, M., Fürst, F., Schwarm, F., Kreykenbohm, I., Wilms, J., Schönherr, G., Caballero, I., Camero-Arranz, A., Bodaghee, A., Doroshenko, V., Klochkov, D., Santangelo, A., Staubert, R., Kretschmar, P., Wilson-Hodge, C., Finger, M. H., Terada, Y.
Seventeen accreting neutron star pulsars, mostly high mass X-ray binaries with half of them Be-type transients, are known to exhibit Cyclotron Resonance Scattering Features (CRSFs) in their X-ray spectra, with characteristic line energies from 10 to
Externí odkaz:
http://arxiv.org/abs/1111.1800
Autor:
Fuerst, F., Suchy, S., Kreykenbohm, I., Barragan, L., Wilms, J., Pottschmidt, K., Caballero, I., Kretschmar, P., Ferrigno, C., Rothschild, R. E.
Publikováno v:
A&A 535 (2011) A9
We present an in-depth study of the High Mass X-ray Binary (HMXB) GX 301-2 during its pre-periastron flare using data from the XMM-Newton satellite. The energy spectrum shows a power law continuum absorbed by a large equivalent hydrogen column on the
Externí odkaz:
http://arxiv.org/abs/1110.2700
Autor:
Caballero, I., Pottschmidt, K., Santangelo, A., Barragan, L., Klochkov, D., Ferrigno, C., Rodriguez, J., Kretschmar, P., Suchy, S., Marcu, D. M., Mueller, D., Wilms, J., Kreykenbohm, I., Rothschild, R. E., Staubert, R., Finger, M. H., Camero-Arranz, A., Makishima, K., Mihara, T., Nakajima, M., Enoto, T., Iwakiri, W., Terada, Y.
The Be/X-ray binary A0535+26 showed a giant outburst in December 2009 that reached ~5.14 Crab in the 15-50 keV range. Unfortunately, due to Sun constraints it could not be observed by most X-ray satellites. The outburst was preceded by four weaker ou
Externí odkaz:
http://arxiv.org/abs/1107.3417
Autor:
Fuerst, F., Kreykenbohm, I., Suchy, S., Barragan, L., Wilms, J., Rothschild, R. E., Pottschmidt, K.
We present the first detailed spectral and timing analysis of the High Mass X-ray Binary (HMXB) 4U 1909+07 with INTEGRAL and RXTE. 4U 1909+07 is detected in the ISGRI 20-40 keV energy band with an average countrate of 2.6 cps. The pulse period of ~60
Externí odkaz:
http://arxiv.org/abs/1011.5052
Autor:
Caballero, I., Pottschmidt, K., Barragan, L., Ferrigno, C., Kretschmar, P., Suchy, S., Wilms, J., Santangelo, A., Kreykenbohm, I., Rothschild, R., Klochkov, D., Staubert, R., Finger, M. H., Camero-Arranz, A., Makishima, K., Mihara, T., Nakajima, M., Enoto, T., Iwakiri, W., Terada, Y.
A normal outburst of the Be/X-ray binary system A0535+26 has taken place in August 2009. It is the fourth in a series of normal outbursts that have occured around the periastron passage of the source, but is unusual by starting at an earlier orbital
Externí odkaz:
http://arxiv.org/abs/1003.2969
Autor:
Fuerst, F., Kreykenbohm, I., Barragán, L., Wilms, J., Rothschild, R. E., Suchy, S., Pottschmidt, K.
We present the first detailed spectral and timing analysis of the High Mass X-ray Binary (HMXB) 4U 1909+07 with INTEGRAL and RXTE. 4U 1909+07 is detected with an average of 2.4cps in ISGRI, but shows flares up to ~50cps. The system shows a pulse peri
Externí odkaz:
http://arxiv.org/abs/0912.3702