A dataset provided by the European Space Agency

Name: A Comprehensive X-ray Study of W51B+C Complex
Published: 2010-04-29T00:00:00Z

Proposal ID	055469
Title	A Comprehensive X-ray Study of W51B+C Complex
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0554690101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0554690501
DOI	https://doi.org/10.5270/esa-tv1azvu
Principal Investigator, PI	Dr Jae-Joon Lee
Abstract	W51 is a Galactic radio complex consist of star forming regions (SFRs; W51A andW51B) and a supernova remnant (SNR; W51C). W51B and C are a particularly usefulopportunity for the study of the interaction between a supernova remnant andstar-forming regions. We propose joint XMM-Newton and Chandra observations ofW51B/C. XMM-Newton will cover W51C where the large field of view and highthroughput of XMM-Newton are ideal, while Chandra observation will cover W51Bwhere superb angular resolution of Chandra is necessary. Our joint program willbe effective to reveal the nature of the pulsar wind nebula, the origin of thecentral emission in SNR W51C, the origin of diffuse X-ray emission in W51B, andthe star-formation history of W51B.
Publications	XMM-Newton observation of the Galactic supernova remnant W51C (G49.1-0.1) \|Sasaki, Manami, Heinitz, Cornelia, et al. \| A&A \| 563-9 \| 2014 \| 2014A&A...563A...9S \| http://ui.adsabs.harvard.edu/#abs/2014A&A...563A...9S 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 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 Supernova remnant W51C: optical and X-ray emission analysis \|Reyes-Iturbide, J., Ram\\u00edrez-Ballinas, I., et al. \| MNRAS \| 516-6055 \| 2022 \| 2022MNRAS.516.6055R \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.516.6055R 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2009-04-08T10:58:21Z/2009-04-09T09:31:16Z
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	2010-04-29T00:00:00Z
Keywords	"cover w51b", "superb angular resolution", "XMM", "supernova remnant", "cover w51c", "star forming region", "diffuse xray emission", "supernova remnant w51c", "central emission", "XMM-Newton", "star formation history", "pulsar wind nebula", "comprehensive xray", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jae-Joon Lee, 2010, 'A Comprehensive X-ray Study of W51B+C Complex', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-tv1azvu