A dataset provided by the European Space Agency

Name: The dwarfs of the Ring: Star Formation around Kappa Ori explored with XMM-Newton
Published: 2016-04-14T22:00:00Z

Proposal ID	074057
Title	The dwarfs of the Ring: Star Formation around Kappa Ori explored with XMM-Newton
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0740570101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0740570201
DOI	https://doi.org/10.5270/esa-2nj9fbv
Principal Investigator, PI	Dr Ignazio Pillitteri
Abstract	One of the mechanisms proposed for causing the collapse of a gas cloud and startstar formation is the action of an external agent that can compress the gas andcreate the primordial protostellar cores (Elmegreen 1998). While supernovae arethe most dramatic agents, stellar winds from massive stars and the expansion ofionized HII bubbles may play an important role. They can transfer momentum,kinetic energy and heat a close-by gas cloud. A few cases have been identifiedwhere massive stars are responsible of triggered star formation (RCW79, Zavagnoet al. 2006, Sharpless 104, Deharveng et al., 2003). With this XMM proposal, weaim to understand the interaction at work between one single massive star, KappaOri, and Lynds 1641 (L1641), the filamentary cloud in the southern part of the Orion~A cloud.
Publications	A Star-forming Ring around kappa Ori 250 pc from the Sun \|Pillitteri I. Wolk S. J. \| ApJ \| 820-28 \| 2016 \| 2016ApJ...820L..28P \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...820L..28P 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 XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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	2015-03-10T05:34:45Z/2015-03-15T20:57:52Z
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	2016-04-14T22:00:00Z
Last Update	2025-01-27
Keywords	"deharveng .", "xmm newton", "sharpless 104", "kappa ori explored", "single massive star", "ionized hii bubbles", "start star formation", "kinetic energy", "XMM-Newton", "gas cloud", " 2003", "transfer momentum", "stellar winds", "kappa ori", "star formation", "external agent", "filamentary cloud", "lynds 1641 l1641", "XMM", "massive stars"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ignazio Pillitteri, 2016, 'The dwarfs of the Ring: Star Formation around Kappa Ori explored with XMM-Newton', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-2nj9fbv