|Title||Turnoff of H-burning and recovery of accretion in 3 novae detected by XMM|
|Author||Dr Margarita Hernanz|
|Description||Detection of X-rays from classical novae in their post-outburst stages provides unique and crucial information about the explosion mechanism and the re establishment of accretion. Soft X-rays reveal if H-nuclear burning is still on, whereas harder X-rays give diagnostics about the ejecta or the properties of the reborn CV. We have detected 3 interesting novae with our monitoring campaign with XMM in AO6. V5116 Sgr (2005) and V5115 Sgr (2005) were still in the supersoft X-ray phase, with V5116 Sgr displaying a puzzling temporal varibility. V2362 Cyg, on the contrary, had already turned-off, but the short effective exposure (due to high radiation) prevented to disentangle the origin of the emission. We propose new observations of these exciting post-novae.|
|Publication||Swift X-Ray Observations of Classical Novae. II. The Super Soft Source Sample . Schwarz, Greg J., Ness, Jan-Uwe, et all. . ApJS . 197-31 . 2011 . 2011ApJS..197...31S ,
X-ray observations of classical novae: Theoretical implications . Hernanz, M., Sala, G., . AN . 331-169 . 2010 . 2010AN....331..169H ,
V5116 Sgr: A disc-eclipsed SSS post-outburst nova? . Sala, G., Hernanz, M., et all. . AN . 331-201 . 2010 . 2010AN....331..201S ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H ,
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 Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo . Miller, Matthew J., Bregman, Joel N., . ApJ . 829-9 . 2016 . 2016ApJ...829....9M ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
|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, 2010-04-28T00:00:00Z, 055019, 17.56_20190403_1200. https://doi.org/10.5270/esa-o8i7f22|