Zobrazeno 1 - 10
of 38
pro vyhledávání: '"Guillermo Bernabeu"'
Autor:
Jose M. Torrejon, Konstantin Postnov, Guillermo Bernabeu, G Sanjurjo-Ferrín, Lida Oskinova, J. J. Rodes-Roca
Publikováno v:
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Universidad de Alicante (UA)
Cen X−3 is a compact high-mass X-ray binary likely powered by Roche lobe overflow. We present a phase-resolved X-ray spectral and timing analysis of two pointed XMM–Newton observations. The first one took place during a normal state of the source
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::50c6e7ee2e47ffed85f6ade1d17b6f24
http://hdl.handle.net/10045/114151
http://hdl.handle.net/10045/114151
Publikováno v:
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Universidad de Alicante (UA)
The aim of this work is to characterize the counterpart to the INTEGRAL High Mass X-ray Binary candidate IGR J19294+1816 so as to establish its true nature. We obtained H band spectra of the selected counterpart acquired with the NICS instrument moun
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a8bdc3db5b5f80a940034e1a3c127f8d
Autor:
Jose M. Torrejon, Guillermo Bernabeu, G. Sanjurjo-Ferrrín, Konstantin Postnov, Lida Oskinova, J. J. Rodes-Roca
Publikováno v:
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Universidad de Alicante (UA)
Aims. 4U0114+65 is one of the slowest known X-ray pulsars. We present an analysis of a pointed observation by the XMM-Newton X-ray telescope in order to study the nature of the X-ray pulsations and the accretion process, and to diagnose the physical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e2cbbcae88677bd6035f447da4643558
https://publishup.uni-potsdam.de/frontdoor/index/index/docId/46248
https://publishup.uni-potsdam.de/frontdoor/index/index/docId/46248
Publikováno v:
Astronomische Nachrichten. 335:804-811
This work was supported by the Spanish Ministry of Education and Science “De INTEGRAL a IXO: binarias de rayos X y estrellas activas”, project number AYA2010-15431, partially by GV2014/088 and MIF/14G04. JJRR acknowledges the support by the Spani
Autor:
S. Martínez-Núñez, Jose M. Torrejon, Lidia M. Oskinova, J. Alonso-Santiago, Andreas Sander, Carlos González-Fernández, Guillermo Bernabeu, A. Giménez-García, Tomer Shenar, A. Gonzalez-Galan, J. J. Rodes-Roca, Wolf-Rainer Hamann
Publikováno v:
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Universidad de Alicante (UA)
Digital.CSIC. Repositorio Institucional del CSIC
instname
[Context]: Classical supergiant X-ray binaries (SGXBs) and supergiant fast X-ray transients (SFXTs) are two types of high-mass X-ray binaries (HMXBs) that present similar donors but, at the same time, show very different behavior in the X-rays. The r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::994de6e810eb76f622eee9063862af4a
Publikováno v:
European Journal of Physics. 31:L65-L70
A closed-form approximate expression for the solution of a simple pendulum in terms of elementary functions is obtained. To do this, the exact expression for the maximum tension of the string of the pendulum is first considered and a trial approximat
Autor:
J. J. Rodes-Roca, Satoshi Nakahira, Guillermo Bernabeu, Jose M. Torrejon, Tatehiro Mihara, Angel Gímenez-García
Publikováno v:
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Universidad de Alicante (UA)
4U 1538-52, an absorbed high mass X-ray binary with an orbital period of 3.73 days, shows moderate orbital intensity modulations with a low level of counts during the eclipse. Several models have been proposed to explain the accretion at different or
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::819b46314a7da46649fcc86d54fe2d46
http://hdl.handle.net/10045/49045
http://hdl.handle.net/10045/49045
Autor:
Angel Gímenez-García, Jose M. Torrejon, J. J. Rodes-Roca, S. Martínez-Núñez, Guillermo Bernabeu, Lida Oskinova, W. Eikmann
Publikováno v:
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Universidad de Alicante (UA)
We present a comprehensive analysis of the whole sample of available XMM-Newton observations of high-mass X-ray binaries (HMXBs) until August 2013, focusing on the FeKα emission line. This line is key to better understanding the physical properties
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::85f0ad3344c23d4dded43d2564b1bb84
http://hdl.handle.net/10045/46265
http://hdl.handle.net/10045/46265
Autor:
Hans Jochen Scholl, Jj Kavelaars, M. Holman, P. Rousselot, O. Mousis, T. Grav, Paula Gabriela Benavídez, P. D. Nicholson, Brett Gladman, J. Wm. Parker, Jean-Marc Petit, R. L. Jones, A. Campo Bagatin, C. Veillet, G. Mars, Alain Doressoundiram, Guillermo Bernabeu
Publikováno v:
Icarus
Icarus, Elsevier, 2006, 185, pp.508-522. ⟨10.1016/j.icarus.2006.07.024⟩
Icarus, Elsevier, 2006, 185 (2), pp.508-522. ⟨10.1016/j.icarus.2006.07.024⟩
Icarus, 2006, 185 (2), pp.508-522. ⟨10.1016/j.icarus.2006.07.024⟩
Icarus, 2006, 185, pp.508-522. ⟨10.1016/j.icarus.2006.07.024⟩
Icarus, Elsevier, 2006, 185, pp.508-522. ⟨10.1016/j.icarus.2006.07.024⟩
Icarus, Elsevier, 2006, 185 (2), pp.508-522. ⟨10.1016/j.icarus.2006.07.024⟩
Icarus, 2006, 185 (2), pp.508-522. ⟨10.1016/j.icarus.2006.07.024⟩
Icarus, 2006, 185, pp.508-522. ⟨10.1016/j.icarus.2006.07.024⟩
We present the data acquisition strategy and characterization procedures for the Canada-France Ecliptic Plane Survey (CFEPS), a sub-component of the Canada-France-Hawaii Telescope Legacy Survey. The survey began in early 2003 and as of summer 2005 ha
Autor:
Guillermo Bernabeu, Amparo Marco
Publikováno v:
Astronomy & Astrophysics. 372:477-494
We present uvby CCD photometry of the central region of the double cluster h & Persei. We identify 350 stars, of which 214 were not included in Oosterhof's catalogue. Our magnitude limit V =1 6:5 allows us to reach early F spectral type and obtain ve