A dataset provided by the European Space Agency

Name 050374
Title A First X-ray View of Infrared Dark Clouds, Precursors to Star Clusters
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503740101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503740201

DOI 10.5270/esa-38i990p
Author Mr Junfeng Wang
Description A large population of infrared dark clouds (IRDCs) was recently discovered as a new component of the cold interstellar medium, inside which infrared and radio studies provide evidence for massive star formation. They are thought to represent the earliest phases of the formation of star clusters and massive stars. We propose to observe one of the closest massive IRDCs with XMM-Newton, as the first X-ray study of this new population of objects. This 84 ks EPIC observation of G053.11+00.05 will quantitatively measure the embedded stellar populations, especially the low mass stars that XMM-Newton effectively identifies. The goals are to evaluate the roles of IRDCs in the formation of star clusters and massive stars, and to constrain the current theories of clustered massive star formation.
Publication Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
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 ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Investigating Galactic Supernova Remnant Candidates Using LOFAR . Driessen, Laura N., Domcek, Vladimir, et all. . ApJ . 860-133 . 2018 . 2018ApJ...860..133D ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-03-29T12:34:28Z/2008-03-30T06:40:19Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2009-06-05T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-06-05T00:00:00Z, 050374, 17.56_20190403_1200. https://doi.org/10.5270/esa-38i990p