|Title||A time-resolved study of the injection of mass onto a dormant Supermassive Black|
|Author||Mr Richard Saxton|
|Description||The near real-time comparison of XMM-Newton slew data with the ROSAT all-sky survey gives an excellent opportunity to find black holes in the centres of galaxies, which are currently being fueled by the tidal disruption of a star. In June 2010, as part of this program, we detected a flare from the optically quiescent galaxy SDSS J120136.02+300305.5 and monitored its evolution. The source flux decays at the rate predicted for returning tidal debris but with surprisingly strong variations. A factor 50 flux reduction seen after 30 days, could be due to absorption by a super-Eddington outflow or may be caused by jet instabilities. We propose to extend this program to find and monitor more candidates and ultimately produce a small sample which can address the physics of tidal disruption events.|
|Publication||An X-ray and UV flare from the galaxy XMMSL1 J061927.1-655311 . Saxton, R. D., Read, A. M., et all. . A&A . 572-1 . 2014 . 2014A&A...572A...1S ,
The population of X-ray supernova remnants in the Large Magellanic Cloud . Maggi, P., Haberl, F., et all. . A&A . 585-162 . 2016 . 2016A&A...585A.162M ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Identification of high-mass X-ray binaries selected from XMM-Newton observations of the LMC* . van Jaarsveld, N., Buckley, D. A. H., et all. . MNRAS . 475-3253 . 2018 . 2018MNRAS.475.3253V ,
Physics and observations of tidal disruption events . Mangalam, Arun, Mageshwaran, Tamilan, . BSRSL . 87-307 . 2018 . 2018BSRSL..87..307M ,
X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC . Ou, Po-Sheng, Chu, You-Hua, et all. . ApJ . 863-137 . 2018 . 2018ApJ...863..137O ,
New optically identified supernova remnants in the Large Magellanic Cloud . Yew, Miranda, Filipoviu0107, Miroslav D., et all. . MNRAS . 500-2336 . 2021 . 2021MNRAS.500.2336Y ,
|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, 2014-05-04T00:00:00Z, 069110, 17.56_20190403_1200. https://doi.org/10.5270/esa-tsnpjt1|