A dataset provided by the European Space Agency

Name: Portrait of a Giant HII Bubble: Star Formation Processes in the Cepheus Loop
Published: 2014-01-19T00:00:00Z

Proposal ID	070099
Title	Portrait of a Giant HII Bubble: Star Formation Processes in the Cepheus Loop
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700990101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700990201
DOI	https://doi.org/10.5270/esa-uptk6tp
Principal Investigator, PI	Dr Konstantin Getman
Abstract	We propose to study star formation associated with giant, asymmetric HII bubblesvia three observations of the nearby bubble Cepheus Loop. An ACIS-I GO pointing(50ks) will characterize the rich and compact principal ionizing cluster Be59.XMM EPIC/pn pointings (2x30ks) will search for low-mass members of a suspectedolder generation of stars that could have both carved the Cepheus Loop andinduced the formation of Be59, testing an important model for the morphology andevolution of asymmetric bubbles.
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	2012-12-30T20:47:31Z/2012-12-31T15:49:25Z
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	2014-01-19T00:00:00Z
Keywords	"star formation", "xmm epic", "XMM", "low mass", "asymmetric bubbles", "giant hii bubble", "star formation processes", "cepheus loop", "EPIC", "pn pointings 2x30"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Konstantin Getman, 2014, 'Portrait of a Giant HII Bubble: Star Formation Processes in the Cepheus Loop', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-uptk6tp