A dataset provided by the European Space Agency

Name: Joint Chandra/XMM/EVLA Monitoring of the Gas Cloud G2 as it encounters SGR A*
Published: 2014-09-26T00:00:00Z

Proposal ID	070098
Title	Joint Chandra/XMM/EVLA Monitoring of the Gas Cloud G2 as it encounters SGR A*
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700980101
DOI	https://doi.org/10.5270/esa-8nx58e5
Principal Investigator, PI	Dr Daryl Haggard
Abstract	A dense, cold cloud (G2) is on a collision course with Sgr A, the radio sourceat our Galactic Center. G2 is on an eccentric orbit and already shows signs oftidal disruption by the black hole. High-energy emission from Sgr A will likelyincrease significantly due to this encounter, peaking at pericenter (summer2013). We propose simultaneous Chandra, XMM, and EVLA monitoring observations toconstrain the rates and emission mechanisms of faint X-ray flares, study theradiation properties of Sgr A* as G2 breaks up and feeds gas to the centralaccretion flow, and detect G2 itself as it is shocked and heated.
Publications	On the Fe K absorption - accretion state connection in the Galactic Centre neutron star X-ray binary AX J1745.6-2901 \|Ponti G. Bianchi S. et al. \| MNRAS \| 446-1536 \| 2015 \| 2015MNRAS.446.1536P \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.446.1536P The X-ray outburst of the Galactic Centre magnetar SGR J1745-2900 during the first 1.5 year \|Coti Zelati F. Rea N. et al. \| MNRAS \| 449-2685 \| 2015 \| 2015MNRAS.449.2685C \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.449.2685C Fifteen years of XMM-Newton and Chandra monitoring of Sgr A: evidence for a recent increase in the bright flaring rate \|Ponti G. De Marco B. et al. \| MNRAS \| 454-1525 \| 2015 \| 2015MNRAS.454.1525P \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.454.1525P High ionisation absorption in low mass X-ray binaries \|Ponti G. Bianchi S. et al. \| AN \| 337-512 \| 2016 \| 2016AN....337..512P \| http://ui.adsabs.harvard.edu/#abs/2016AN....337..512P The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F The puzzling orbital period evolution of the LMXB AX J1745.6-2901 \|Ponti G. De K. et al. \| MNRAS \| 464-840 \| 2017 \| 2017MNRAS.464..840P \| http://ui.adsabs.harvard.edu/#abs/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 al. \| MNRAS \| 465-45 \| 2017 \| 2017MNRAS.465...45C \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.465...45C Polarization and long-term variability of Sgr A* X-ray echo \|Churazov E. Khabibullin I. et al. \| MNRAS \| 468-165 \| 2017 \| 2017MNRAS.468..165C \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/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 al. \| MNRAS \| 468-2532 \| 2017 \| 2017MNRAS.468.2532J \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.468.2532J Chandra monitoring of the Galactic Centre magnetar SGR J1745-2900 during the initial 3.5 years of outburst decay \|Coti Zelati F. Rea N. et al. \| MNRAS \| 471-1819 \| 2017 \| 2017MNRAS.471.1819C \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.1819C Can Sgr A flares reveal the molecular gas density PDF? \|Churazov E. Khabibullin I. et al. \| MNRAS \| 471-3293 \| 2017 \| 2017MNRAS.471.3293C \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.3293C A transient flat spectrum radio pulsar near the Galactic Centre \|Dexter J. Degenaar N. et al. \| MNRAS \| 468-1486 \| 2017 \| 2017MNRAS.468.1486D \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.468.1486D A 149 min periodicity underlies the X-ray flaring of Sgr A* \|Leibowitz Elia \| MNRAS \| 474-3380 \| 2018 \| 2018MNRAS.474.3380L \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.474.3380L Effects of interstellar dust scattering on the X-ray eclipses of the LMXB AX J1745.6-2901 in the Galactic Centre \|Jin Chichuan Ponti Gabriele et al. \| MNRAS \| 477-3480 \| 2018 \| 2018MNRAS.477.3480J \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.477.3480J X-ray chimneys in the Galactic Centre \|Chernyakova Masha \| Natur \| 567-318 \| 2019 \| 2019Natur.567..318C \| http://ui.adsabs.harvard.edu/#abs/2019Natur.567..318C An X-ray chimney extending hundreds of parsecs above and below the Galactic Centre \|Ponti G. Hofmann F. et al. \| Natur \| 567-347 \| 2019 \| 2019Natur.567..347P \| http://ui.adsabs.harvard.edu/#abs/2019Natur.567..347P A Rapidly Varying Red Supergiant X-Ray Binary in the Galactic Center \|Gottlieb Amy M. Eikenberry Stephen S. et al. \| ApJ \| 896-32 \| 2020 \| 2020ApJ...896...32G \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...32G The Galactic center chimneys: the base of the multiphase outflow of the Milky Way \|Ponti G. Morris M. R. et al. \| A&A \| 646-66 \| 2021 \| 2021A&A...646A..66P \| http://ui.adsabs.harvard.edu/#abs/2021A&A...646A..66P Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Tracing the Milky Ways Vestigial Nuclear Jet \|Cecil Gerald Wagner Alexander Y. et al. \| ApJ \| 922-254 \| 2021 \| 2021ApJ...922..254C \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...922..254C SRG/eROSITA view of X-ray reflection in the Central Molecular Zone: a snapshot in September-October 2019 \|Khabibullin Ildar Churazov Eugene \| MNRAS \| 509-6068 \| 2022 \| 2022MNRAS.509.6068K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.6068K The episodic and multiscale Galactic Centre \|Bryant Aaron Krabbe Alfred \| NewAR \| 93-101630 \| 2021 \| 2021NewAR..9301630B \| http://ui.adsabs.harvard.edu/#abs/2021NewAR..9301630B Constraining particle acceleration in Sgr A^u22c6 with simultaneous GRAVITY Spitzer NuSTAR and Chandra observations \|GRAVITY Collaboration Abuter R. et al. \| A&A \| 654-22 \| 2021 \| 2021A&A...654A..22G \| http://ui.adsabs.harvard.edu/#abs/2021A&A...654A..22G X-ray astronomy comes of age \|Wilkes Belinda J. Tucker Wallace et al. \| Natur \| 606-261 \| 2022 \| 2022Natur.606..261W \| http://ui.adsabs.harvard.edu/#abs/2022Natur.606..261W X-ray polarization evidence for a 200-year-old flare of Sgr A^* \|Marin Fru00e9du00e9ric Churazov Eugene et al. \| Natur \| 619-41 \| 2023 \| 2023Natur.619...41M \| http://ui.adsabs.harvard.edu/#abs/2023Natur.619...41M Scientific objectives of the Hot Universe Baryon Surveyor (HUBS) mission \|Bregman Joel Cen Renyue et al. \| SCPMA \| 66-299513 \| 2023 \| 2023SCPMA..6699513B \| http://ui.adsabs.harvard.edu/#abs/2023SCPMA..6699513B The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way \|Sarkar Kartick C. \| A&ARv \| 32-1 \| 2024 \| 2024A&ARv..32....1S \| http://ui.adsabs.harvard.edu/#abs/2024A&ARv..32....1S Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2013-09-10T03:30:45Z/2013-09-10T14:15:45Z
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	2014-09-26T00:00:00Z
Last Update	2025-01-27
Keywords	"eccentric orbit", "g2 brea", "cold cloud g2", "pericenter summer 2013", "emission mechanisms", "encounters sgr", "tidal disruption", "radio source", "energy emission", "galactic center", "collision course", "XMM", "feeds gas", "central accretion flow", "gas cloud g2", "radiation properties", "black hole", "faint xray flares"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Daryl Haggard, 2014, 'Joint Chandra/XMM/EVLA Monitoring of the Gas Cloud G2 as it encounters SGR A*', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-8nx58e5