A dataset provided by the European Space Agency

Name: Nature of a Maser-Emitting and EGRET Source SNR: SNR-Molecular Cloud Interaction
Published: 2007-05-31T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	030651
Title	Nature of a Maser-Emitting and EGRET Source SNR: SNR-Molecular Cloud Interaction
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0306510101
DOI	https://doi.org/10.5270/esa-yn0lcz1
Principal Investigator, PI	Mr Hiroshi Nakajima
Abstract	The interaction between SNRs and molecular clouds causes immediate heating andchanges the chemical composition of the surrounding gas, emitting thermal andnon-thermal X-rays, OH maser lines, and gamma-rays. However, what causes thepartial overlap among maser-emitting SNRs, EGRET source SNRs, SNRs withparticular X-ray properties such as mixed-morphology SNRs is still unclear. CTB37A is a radio-bright Galactic SNR, and is accompanied by OH masers and EGRETsource. As the best target for the study of the SNRs in the dense conditions, wepropose the wide-band and large effective area observation of CTB 37A withXMM-Newton.
Publications	Discovery of a VHE gamma-ray source coincident with the supernova remnant CTB 37A \|Aharonian F. Akhperjanian A. G. et al. \| A&A \| 490-685 \| 2008 \| 2008A&A...490..685A \| http://ui.adsabs.harvard.edu/#abs/2008A&A...490..685A The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens Nicola Romer A. Kathy et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies E. J. Romer A. Kathy et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L The X-Ray Properties of Five Galactic Supernova Remnants Detected by the Spitzer GLIMPSE Survey \|Pannuti Thomas G. Rho Jeonghee et al. \| AJ \| 147-55 \| 2014 \| 2014AJ....147...55P \| http://ui.adsabs.harvard.edu/#abs/2014AJ....147...55P 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 Sunyaev-Zeldovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao Weike Chen Chen et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X 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 A view of supernova remnant CTB 37A with the Fermi Gamma-ray Space Telescope \|Brandt T. J. Fermi-LAT Collaboration \| AdSpR \| 51-247 \| 2013 \| 2013AdSpR..51..247B \| http://ui.adsabs.harvard.edu/#abs/2013AdSpR..51..247B Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas Konstantinos Reiprich Thomas H. \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The XMM Cluster Survey: Present status and latest results \|Viana P. T. P. Mehrtens N. et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V Testing emergent gravity on galaxy cluster scales \|Tamosiunas Andrius Bacon David et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood Devon L. Jeltema Tesla et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese A. Annis J. et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P 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	2006-03-01T14:22:24Z/2006-03-01T19:09:24Z
Version	21.51_20241115_1113
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	2007-05-31T00:00:00Z
Last Update	2026-07-09
Keywords	"wide band", "XMM-Newton", "emitting thermal", "egret source", "oh masers", "dense conditions", "molecular clouds causes", "maser emitting", "xray properties", "supernova remnant", "nonthermal xray", "XMM", "partial overlap", "oh maser lines", "ctb 37a", "chemical composition", "gamma rays", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Hiroshi Nakajima, 2007, 'Nature of a Maser-Emitting and EGRET Source SNR: SNR-Molecular Cloud Interaction', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-yn0lcz1
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.