A dataset provided by the European Space Agency

Name 060607
Title A deep look at accretion disks: Fe lines, kHz QPOs and spectral states.


DOI 10.5270/esa-prj8otg
Description Iron lines have now been detected in about half a dozen neutron-star accreting X-ray binaries. These lines can be used to set tight constrains on the accretion disk geometry and on the radius of the neutron star. We have recently shown that simultaneous XMM-Newton-RXTE and Chandra-RXTE observations appear to contradict previous works. Here we propose to observe a NS with XMM-Newton seven times for 25~ks, simultaneously with some of those RXTE observations. Our program will sample a wide range of inner disk radii. This program requires both XMM-Newton and RXTE observations. Since 2009 may be the last year of operations of RXTE, this program can only be done now.
Publication Interstellar medium composition through X-ray spectroscopy of low-mass X-ray binaries . Pinto, C., Kaastra, J. S., et all. . A&A . 551-25 . 2013 . 2013A&A...551A..25P ,
Broad iron line in the fast spinning neutron-star system 4U 1636-53 . Sanna, Andrea, Hiemstra, Beike, et all. . MNRAS . 432-1144 . 2013 . 2013MNRAS.432.1144S ,
Iron-line and continuum variations in the XMM-Newton and Suzaku spectra of the neutron-star low-mass X-ray binary 4U 1636-53 . Lyu, Ming, Mendez, Mariano, et all. . MNRAS . 440-1165 . 2014 . 2014MNRAS.440.1165L ,
Broad iron emission line and kilohertz quasi-periodic oscillations in the neutron star system 4U 1636-53 . Sanna, Andrea, Mendez, Mariano, et all. . MNRAS . 440-3275 . 2014 . 2014MNRAS.440.3275S ,
Discovery of a correlation between the frequency of the mHz quasi-periodic oscillations and the neutron-star temperature in the low-mass X-ray binary 4U 1636-53 . Lyu, Ming, Mendez, Mariano, . MNRAS . 445-3659 . 2014 . 2014MNRAS.445.3659L ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Spectral and timing analysis of the mHz QPOs in the neutron-star low-mass X-ray binary 4U 1636-53 . Lyu, Ming, Mendez, Mariano, et all. . MNRAS . 454-541 . 2015 . 2015MNRAS.454..541L ,
Oxygen, neon, and iron X-ray absorption in the local interstellar medium . Gatu...
Instrument EPN, OM, RGS1, RGS2
Temporal Coverage 2009-03-14T14:50:30Z/2009-09-11T16:01:56Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2010-10-27T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-10-27T00:00:00Z, 060607, 17.56_20190403_1200. https://doi.org/10.5270/esa-prj8otg