A dataset provided by the European Space Agency

Proposal ID 074363
Title Monitoring a close encounter between a small cloud and a supermassive BH
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743630201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743630301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743630401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743630501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743630601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743630701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743630801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743630901

DOI https://doi.org/10.5270/esa-dt0hzik
Principal Investigator, PI Dr Gabriele Ponti
Abstract A gas cloud, dubbed G2, was recently discovered to be falling towards Sgr A*.This allows us to witness the unique occurrence of a cloud interacting with theBH.s close environment and likely partially accreting. We propose 4*50 ks XMMobservations to: i) monitor the long term variations of the X-ray flux producedby Sgr A* as it interacts with the cloud; ii) monitor any variation, induced bythe cloud flyby, to the frequency and intensity of Sgr A*.s flaring activity;iii) use the magnetar.s light echo and its variations to scan the Galacticcentre matter distribution around Sgr A*; iv) monitor the evolution of thesuperluminal echo reflected from the Bridge.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2014-08-30T19:20:01Z/2015-04-02T19:04:19Z
Version 17.56_20190403_1200
Mission Description The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 2016-05-06T22:00:00Z
Keywords "", "XMM", "partially accreting", "xray flux", "flaring activity", "dubbed g2", "superluminal echo reflected", "light echo"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Gabriele Ponti, 2016, 'Monitoring a close encounter between a small cloud and a supermassive BH', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-dt0hzik