A dataset provided by the European Space Agency

Name: X-ray diving in the center of Sh2-129: looking for the driving source of Ou4
Published: 2014-08-31T00:00:00Z

Proposal ID	072230
Title	X-ray diving in the center of Sh2-129: looking for the driving source of Ou4
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722300101
DOI	https://doi.org/10.5270/esa-sofh816
Principal Investigator, PI	Dr Nicolas Grosso
Abstract	The outflow phenomenon is associated both with the early and the last phase ofthe stellar evolution. Recently, a unique bipolar outflow with an angular sizeof 1.2 degrees was discovered in the blister HII region Sh2-129. Ou4, nicknamedThe Giant Squid, is to our knowledge the bipolar outflow with the largestangular size ever found. We propose joint XMM-Newton/EPIC (35 ks) andChandra/HRC-I (16 ks) observations to look for the driving source of Ou4 and toclarify the nature of this object.
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 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	2013-07-27T00:49:40Z/2013-07-27T13:18:00Z
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	2014-08-31T00:00:00Z
Last Update	2025-01-27
Keywords	"", "EPIC", "sh2 129", "outflow phenomenon", "xmm newton", "XMM-Newton", "giant squid "", "largest angular size", "stellar evolution", "driving source", "angular size", "XMM", "bipolar outflow", "x ray diving"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Nicolas Grosso, 2014, 'X-ray diving in the center of Sh2-129: looking for the driving source of Ou4', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-sofh816