A dataset provided by the European Space Agency

Name: Newly-Discovered Regions of Star Formation in Serpens and Perseus
Published: 2009-06-10T00:00:00Z

Proposal ID	050324
Title	Newly-Discovered Regions of Star Formation in Serpens and Perseus
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503240201
DOI	https://doi.org/10.5270/esa-dkaucsv
Principal Investigator, PI	Dr Geoffrey Blake
Abstract	We shall obtain EPIC observations of two fields in Serpens centered on newlydiscovered regions of recent star formation. Spitzer IR maps of these regionsreveal dense molecular gas and numerous previously unknown PMS stars, diverse inboth mass and age. Comparison of the IR disk and X-ray coronal properties willallow detailed characterization of the individual stars and investigation ofevolutionary trends in different regions. Young stars are strong X-ray emittersthroughout their PMS evolution, from embedded protostars to older dust-free (andhence IR-faint) PMS stars. X-ray emission provides an excellent method oftracing the entire PMS population and investigating the star formation historiesof these regions and the processes controlling the fragmentation and formation of stars.
Publications	An All-Sky Atlas of Radio/X-ray Associations \|Flesch E. \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin Dacheng Webb Natalie A. \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L The diversity of quasars unified by accretion and orientation \|Shen Yue Ho Luis C. \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S 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 New X-Ray-selected Pre-main-sequence Members of the Serpens Molecular Cloud \|Oliveira Isa van der Laan Margriet \| AJ \| 146-105 \| 2013 \| 2013AJ....146..105O \| http://ui.adsabs.harvard.edu/#abs/2013AJ....146..105O 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	2008-04-16T17:32:13Z/2008-04-17T07:57:29Z
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	2009-06-10T00:00:00Z
Last Update	2025-01-27
Keywords	"dense molecular gas", "EPIC", "xray coronal properties", "pms population", "star formation histories", "star formation", "pms evolution", "spitzer ir maps", "serpens centered", "processes controlling", "evolutionary trends", "dust free", "pms stars", "embedded protostars", "xray emission", "ir disk", "xray emitters throughout", "individual stars"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Geoffrey Blake, 2009, 'Newly-Discovered Regions of Star Formation in Serpens and Perseus', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-dkaucsv