A dataset provided by the European Space Agency

Name: Probing Environmental Effect on CIrcumstellar Disk Evolution: the W3,W4 complex
Published: 2014-03-09T00:00:00Z

Proposal ID	069208
Title	Probing Environmental Effect on CIrcumstellar Disk Evolution: the W3,W4 complex
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692080201
DOI	https://doi.org/10.5270/esa-0hzx8kb
Principal Investigator, PI	Dr Jinyoung Serena Kim
Abstract	We propose XMM/EPIC & Chandra/ACIS-I observations for the W3,W4 star formingregions to study circumstellar disk evolution in a high radiation environment.Multi-wavelength studies are necessary to obtain unbiased samples of young starsfor statistical analysis: IR excess emission identifies stars with disks whileX-rays help find diskless young stars. A candidate birth place of our SolarSystem is a high radiation environment in the vicinity of massive stars. We aretesting the hypothesis that planetary systems like our own commonly form in suchhigh radiation environment. With the unbiased sample of young stars from theproposed observations combined with what we have obtained, we will determinedisk frequency as a function of mass and age, and will compare them with different environments.
Publications	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 The value-added catalogue of ASAS-SN eclipsing binaries: parameters of 30 000 detached systems \|Rowan D. M. Jayasinghe T. et al. \| MNRAS \| 517-2190 \| 2022 \| 2022MNRAS.517.2190R \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517.2190R 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	2013-02-23T03:35:25Z/2013-02-23T16:33:59Z
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	2014-03-09T00:00:00Z
Last Update	2025-01-27
Keywords	"unbiased samples", "EPIC", "candidate birth", "unbiased sample", "planetary systems", "solar system", "statistical analysis", "multi wavelength", "massive stars", "XMM", "circumstellar disk evolution", "probing environmental effect", "w4 complex", "own commonly form", "disk frequency"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jinyoung Serena Kim, 2014, 'Probing Environmental Effect on CIrcumstellar Disk Evolution: the W3,W4 complex', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0hzx8kb