A dataset provided by the European Space Agency

Proposal ID 072421
Title Monitoring the close encounter between a small cloud and a supermassive BH
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724210201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724210501

DOI https://doi.org/10.5270/esa-wbpoh3o
Principal Investigator, PI Dr Gabriele Ponti
Abstract Earlier this year a gas cloud was discovered to be falling (accelerating)towards SgrA* and it is predicted to reach peribothron (at 2200 rS) in September2013. At a minimum, the cloud-SgrA* interaction is expected to induce enhancedemission varying on timescales of months/years. However, the cloud physics andSgrA*.s close environment are not well understood. We propose 4*50ks XMMobservations to study the near-future evolution of the cloud. Its emissionproperties will be a sensitive probe of the characteristics of the accretionflow onto the supermassive Galactic BH, at milli-parsec scales.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2013-08-30T20:13:12Z/2013-09-23T09:27:29Z
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 2014-10-10T00:00:00Z
Keywords "close encounter", "emission properties", "XMM", "cloud sgra", "supermassive bh", "cloud physics", "future evolution", "milli parsec scales", "2200 rs", "gas cloud", "sgra *'", "supermassive galactic bh", "september 2013", "sensitive probe", "accretion flow", "accelerating towards sgra"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Gabriele Ponti, 2014, 'Monitoring the close encounter between a small cloud and a supermassive BH', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-wbpoh3o