A dataset provided by the European Space Agency

Name: A twin cluster to Collinder 69 in the lambda Orionis star forming region
Published: 2010-09-22T00:00:00Z

Proposal ID	060212
Title	A twin cluster to Collinder 69 in the lambda Orionis star forming region
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602120101
DOI	https://doi.org/10.5270/esa-toh4srj
Principal Investigator, PI	Dr Beate Stelzer
Abstract	The lambda Ori star forming region (5 Myr, 400 pc) is surrounded by a 5 x 5 degwide molecular ring probably formed by a supernova explosion. Our previousmulti-wavelength studies focused on the most well-known areas within the cloudcomplex. For a complete picture of star formation, believed to be determined bythe supernova blast, the large-scale distribution of the pre-main sequencepopulation in lambda Ori needs to be examined. We suspect a further pre-mainsequence cluster to be associated with a concentration of B-type stars near theNE of the molecular ring. A search for X-ray emission is the most efficient wayof identifying the low-mass cluster. The properties of its members will then becompared to the other lambda Ori subgroups.
Publications	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 A new multiwavelength census of blazars \|Paggi A. Bonato M. et al. \| A&A \| 641-62 \| 2020 \| 2020A&A...641A..62P \| http://ui.adsabs.harvard.edu/#abs/2020A&A...641A..62P 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	2009-09-05T23:06:37Z/2009-09-06T13:32:08Z
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	2010-09-22T00:00:00Z
Last Update	2025-01-27
Keywords	"lambda ori subgroups", "twin cluster", "star formation", "type stars", "supernova explosion", "low mass cluster", "scale distribution", "complete picture", "multi wavelength", "xray emission", "lambda ori", "cloud complex", "molecular ring", "supernova blast"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Beate Stelzer, 2010, 'A twin cluster to Collinder 69 in the lambda Orionis star forming region', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-toh4srj