A dataset provided by the European Space Agency

Name: Hot Gas in the Low-Metallicity Star-Forming Small Magellanic Cloud
Published: 2008-03-30T00:00:00Z

Proposal ID	040397
Title	Hot Gas in the Low-Metallicity Star-Forming Small Magellanic Cloud
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0403970301
DOI	https://doi.org/10.5270/esa-ebmwugk
Principal Investigator, PI	Dr Rosa Williams
Abstract	The hot phase of the interstellar medium in a galaxy is produced by the energyfeedback of massive stars. Although the Small Magellanic Cloud (SMC) offers anideal laboratory for the study of hot gas generated by active star formation ina low metallicity environment, there have as yet been few studies of thisdiffuse component. Thus, we propose medium-depth XMM-Newton observations of 5previously unobserved fields along the main body of the SMC. These fieldscontain regions of active star formation. The mechanical energy of stellar windsand supernovae from massive stars have created interstellar structures filledwith hot gas, on a variety of scales. We will analyze the X-ray andmulti-wavelength data to quantitatively assess the stellar energy feedback.
Publications	XMM-Newton observations of the Small Magellanic Cloud: Be/X-ray binary pulsars active between October 2006 and June 2007 \|Haberl F. Eger P. \| A&A \| 489-327 \| 2008 \| 2008A&A...489..327H \| http://ui.adsabs.harvard.edu/#abs/2008A&A...489..327H The XMM-Newton survey of the Small Magellanic Cloud: XMMU J005011.2-730026 = SXP 214 a Be/X-ray binary pulsar \|Coe M. J. Haberl F. et al. \| MNRAS \| 414-3281 \| 2011 \| 2011MNRAS.414.3281C \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.414.3281C High-mass X-ray binary SXP18.3 undergoes the longest type II outburst ever seen in the Small Magellanic Cloud \|Schurch M. P. E. Coe M. J. et al. \| MNRAS \| 392-361 \| 2009 \| 2009MNRAS.392..361S \| http://ui.adsabs.harvard.edu/#abs/2009MNRAS.392..361S 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 Highly absorbed X-ray binaries in the Small Magellanic Cloud \|Novara G. La Palombara N. et al. \| A&A \| 532-153 \| 2011 \| 2011A&A...532A.153N \| http://ui.adsabs.harvard.edu/#abs/2011A&A...532A.153N 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 XMM-Newton survey of the Small Magellanic Cloud \|Haberl F. Sturm R. et al. \| A&A \| 545-128 \| 2012 \| 2012A&A...545A.128H \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A.128H The XMM-Newton survey of the Small Magellanic Cloud: The X-ray point-source catalogue \|Sturm R. Haberl F. et al. \| A&A \| 558-3 \| 2013 \| 2013A&A...558A...3S \| http://ui.adsabs.harvard.edu/#abs/2013A&A...558A...3S Active galactic nuclei behind the SMC selected from radio and X-ray surveys \|Sturm R. Draskovic D. et al. \| A&A \| 558-101 \| 2013 \| 2013A&A...558A.101S \| http://ui.adsabs.harvard.edu/#abs/2013A&A...558A.101S Automatic Classification of Time-variable X-Ray Sources \|Lo Kitty K. Farrell Sean et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L 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 The Role of Stellar Feedback in the Dynamics of H II Regions \|Lopez Laura A. Krumholz Mark R. et al. \| ApJ \| 795-121 \| 2014 \| 2014ApJ...795..121L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...795..121L The Chandra ACIS Timing Survey Project: glimpsing a sample of faint X-ray pulsators \|Israel G. L. Esposito P. et al. \| MNRAS \| 462-4371 \| 2016 \| 2016MNRAS.462.4371I \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.462.4371I Tracing the Lowest Propeller Line in Magellanic High-mass X-Ray Binaries \|Christodoulou Dimitris M. Laycock Silas G. T. et al. \| ApJ \| 829-30 \| 2016 \| 2016ApJ...829...30C \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829...30C 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 Comprehensive Library of X-Ray Pulsars in the Small Magellanic Cloud: Time Evolution of Their Luminosities and Spin Periods \|Yang J. Laycock S. G. T. et al. \| ApJ \| 839-119 \| 2017 \| 2017ApJ...839..119Y \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...839..119Y Retrograde accretion discs in high-mass Be/X-ray binaries \|Christodoulou D. M. Laycock S. G. T. \| MNRAS \| 470-21 \| 2017 \| 2017MNRAS.470L..21C \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470L..21C Deep Chandra Survey of the Small Magellanic Cloud. II. Timing Analysis of X-Ray Pulsars \|Hong JaeSub Antoniou Vallia et al. \| ApJ \| 847-26 \| 2017 \| 2017ApJ...847...26H \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...847...26H The supernova remnant population of the Small Magellanic Cloud \|Maggi Pierre Filipoviu0107 Miroslav D. et al. \| A&A \| 631-127 \| 2019 \| 2019A&A...631A.127M \| http://ui.adsabs.harvard.edu/#abs/2019A&A...631A.127M New optically identified supernova remnants in the Large Magellanic Cloud \|Yew Miranda Filipoviu0107 Miroslav D. et al. \| MNRAS \| 500-2336 \| 2021 \| 2021MNRAS.500.2336Y \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.2336Y 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 Spitzer and Herschel studies of dust in supernova remnants in the Small Magellanic Cloud \|Matsuura Mikako Ayley Victoria et al. \| MNRAS \| 513-1154 \| 2022 \| 2022MNRAS.513.1154M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.1154M The MeerKAT 1.3 GHz Survey of the Small Magellanic Cloud \|Cotton W. D. Filipoviu0107 M. D. et al. \| MNRAS \| 529-2443 \| 2024 \| 2024MNRAS.529.2443C \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.529.2443C 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	2007-03-12T20:01:34Z/2007-03-13T06:53:38Z
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	2008-03-30T00:00:00Z
Last Update	2025-01-27
Keywords	"magellanic cloud", "interstellar medium", "stellar energy feedback", "magellanic cloud smc", "low metallicity", "ideal laboratory", "hot gas", "XMM-Newton", "diffuse component", "main body", "mechanical energy", "massive stars", "XMM", "hot phase", "active star formation", "multi wavelength data", "energy feedback", "stellar winds"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Rosa Williams, 2008, 'Hot Gas in the Low-Metallicity Star-Forming Small Magellanic Cloud', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ebmwugk