A dataset provided by the European Space Agency

Name 072341
Title Monitoring the awakening of the dormant SMBH at the center of our galaxy
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723410301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723410401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723410501

DOI 10.5270/esa-uvn4y0k
Author Dr Nicolas Grosso
Description The recently discovered G2 dense dusty gas cloud, infalling towards the dormant SMBH at the center of our galaxy SgrA*, should reach its pericenter in September 2013. The X-ray luminosity of SgrA* is expected to increase significantly at this period and the fragmentation of this cloud should lead to an enhanced activity period over several months-years. Therefore, we propose a large program to monitor SgrA* during the course of the G2 cloud near its pericenter passage and after this event, combining the XMM-Newton high-throughput with several multi-wavelength observations with ground-based telescopes and satellites. This will offer us an unique opportunity to study accretion events on a dormant SMBH and its (re-)activation process.
Publication Multiwavelength study of the flaring activity of Sagittarius A in 2014 February-April . Mossoux, E., Grosso, N., et all. . A&A . 589-116 . 2016 . 2016A&A...589A.116M ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
The puzzling orbital period evolution of the LMXB AX J1745.6-2901 . Ponti, G., De, K., et all. . MNRAS . 464-840 . 2017 . 2017MNRAS.464..840P ,
Not that long time ago in the nearest galaxy: 3D slice of molecular gas revealed by a 110 yr old flare of Sgr A* . Churazov, E., Khabibullin, I., et all. . MNRAS . 465-45 . 2017 . 2017MNRAS.465...45C ,
Polarization and long-term variability of Sgr A* X-ray echo . Churazov, E., Khabibullin, I., et all. . MNRAS . 468-165 . 2017 . 2017MNRAS.468..165C ,
Sixteen years of X-ray monitoring of Sagittarius A*: Evidence for a decay of the faint flaring rate from 2013 August, 13 months before a rise in the bright flaring rate . Mossoux, Enmanuelle, Grosso, Nicolas, . A&A . 604-85 . 2017 . 2017A&A...604A..85M ,
Probing the interstellar dust towards the Galactic Centre: dust-scattering halo around AX J1745.6-2901 . Jin, Chichuan, Ponti, Gabriele, et all. . MNRAS . 468-2532 . 2017 . 2017MNRAS.468.2532J ,
Can Sgr A* flares reveal the molecular gas density PDF? . Churazov, E., Khabibullin, I., et all. . MNRAS . 471-3293 . 2017 . ...,
NuSTAR + XMM-Newton monitoring of the neutron star transient AX J1745.6-2901 . Ponti, G., Bianchi, S., et all. . MNRAS . 473-2304 . 2018 . 2018MNRAS.473.2304P ,
A transient, flat spectrum radio pulsar near the Galactic Centre . Dexter, J., Degenaar, N., et all. . MNRAS . 468-1486 . 2017 . 2017MNRAS.468.1486D ,
X-ray chimneys in the Galactic Centre . Chernyakova, Masha, . Natur . 567-318 . 2019 . 2019Natur.567..318C ,
An X-ray chimney extending hundreds of parsecs above and below the Galactic Centre . Ponti, G., Hofmann, F., et all. . Natur . 567-347 . 2019 . 2019Natur.567..347P ,
A Rapidly Varying Red Supergiant X-Ray Binary in the Galactic Center . Gottlieb, Amy M., Eikenberry, Stephen S., et all. . ApJ . 896-32 . 2020 . 2020ApJ...896...32G ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2014-02-28T17:41:27Z/2014-04-02T20:29:09Z
Version 17.56_20190403_1200
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.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2015-04-11T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015-04-11T22:00:00Z, 072341, 17.56_20190403_1200. https://doi.org/10.5270/esa-uvn4y0k