|Title||XMM observations of fast spinning HXRTs quiescence|
|Author||Dr Sergio Campana|
|Description||We propose XMM-Newton observations of two hard X--ray transients containing fast spinning and-or high magnetic field neutron stars to probe their quiescent emission. Due to their faintness these sources are likely in a regime which does not allow matter to fall directly onto the neutron star surface (propeller state). The proposed observations will allow us to study 4U 0115+63 and V0332+53 at the deepest levels ever observed for this class of sources to shed light on the physics of the disk-magnetosphere interaction and on the heating of the magnetic polar caps in the high magnetic field regime.|
|Publication||An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
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 ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
The X-ray properties of Be-X-ray pulsars in quiescence . Tsygankov, Sergey S., Wijnands, Rudy, et all. . MNRAS . 470-126 . 2017 . 2017MNRAS.470..126T ,
Recurrent low-level luminosity behaviour after a giant outburst in the Be-X-ray transient 4U 0115+63 . Rouco Escorial, A., Wijnands, R., et all. . A&A . 638-152 . 2020 . 2020A&A...638A.152R ,
|Instrument||EMOS1, EMOS2, EPN, OM, RGS1, RGS2|
|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.
|Publisher And Registrant||European Space Agency|
|Credit Guidelines||European Space Agency, 2008-09-27T00:00:00Z, 050528, 17.56_20190403_1200. https://doi.org/10.5270/esa-xwqsbp5|