A dataset provided by the European Space Agency

Name: X-Ray and Radio Emission of the Galactic Supernova Remnant G7.7-3.7
Published: 2013-04-04T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	067117
Title	X-Ray and Radio Emission of the Galactic Supernova Remnant G7.7-3.7
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671170101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671170201
DOI	https://doi.org/10.5270/esa-2hb3ar6
Principal Investigator, PI	Mr Michael Smith
Abstract	We propose to analyse the X-ray emission of the Galactic SNR G7.7-3.7, a ~21radio SNR with a peculiar filamentary morphology with bright knots. The X-rayemission, as detected by ROSAT and ASCA, seems to be confined to the east of theradio shell, with its intensity increasing at the location of a bright radiofeature near the limb of the SNR and, interestingly, a compact X-ray sourcecoincident with a point-like radio structure. Combining the high quality XMM andradio data will allow us to investigate the nature of the compact X-ray objectand discern between different scenarios which could give rise to the peculiarmorphology. The high spectral and spatial resolution X-ray data covering thecomplete extent of SNR will also be used to constrain its age and energetics.
Publications	Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y 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 G7.7--3.7: A Young Supernova Remnant Probably Associated with the Guest Star in 386 CE (SN 386) \|Zhou Ping Vink Jacco et al. \| ApJ \| 865-6 \| 2018 \| 2018ApJ...865L...6Z \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...865L...6Z 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 From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2012-03-12T08:59:21Z/2012-03-13T03:02:02Z
Version	PPS_NOT_AVAILABLE
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	2013-04-04T00:00:00Z
Last Update	2026-07-09
Keywords	"x ray", "ROSAT", "radio data", "bright radio", "G7.7", "supernova remnant", "filamentary morphology", "XMM", "compact xray object", "radio emission", "quality xmm", "xray emission", "radio shell", "bright knots", "complete extent", "radio supernova remnant", "radio structure"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Michael Smith, 2013, 'X-Ray and Radio Emission of the Galactic Supernova Remnant G7.7-3.7', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-2hb3ar6
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.