A dataset provided by the European Space Agency

Name 055351
Title An XMM-Newton Survey of Rich Open Clusters
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553510101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553510201
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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553510401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553510501
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DOI 10.5270/esa-rercq3l
Author Dr David Pooley
Description We know from observations that globular clusters are efficient catalysts in forming unusual close binary systems and their offspring, and we seek to explore this phenomenon in rich open clusters. We propose a uniform survey of 8 nearby clusters spanning a range of ages and metallicities. The large field of view, high sensitivity, and spatial resolution of XMM are well-matched to such a survey. Similar studies of globulars, undertaken by us, have revealed a link between a cluster.s internal dynamics and its population of X-ray sources. We will examine this link in a regime of stellar density and encounter frequency that is only accessible via the study of open clusters. In addition, UV and U-band photometry will be invaluable to our ongoing studies of open cluster binaries.
Publication An Unexpected Discovery in the Rich Open Cluster NGC 6819 Using XMM-Newton . Gosnell, Natalie M., Pooley, David, et all. . ApJ . 745-57 . 2012 . 2012ApJ...745...57G ,
Estimation of the XUV radiation onto close planets and their evaporation . Sanz-Forcada, J., Micela, G., et all. . A&A . 532-6 . 2011 . 2011A&A...532A...6S ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H ,
Kepler observations of flaring in A-F type stars . Balona, L. A., . MNRAS . 423-3420 . 2012 . 2012MNRAS.423.3420B ,
X-ray emission regimes and rotation sequences in M 35 . An updated model of stellar activity evolution on the main sequence . Gondoin, P., . A&A . 556-14 . 2013 . 2013A&A...556A..14G ,
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 ,
WIYN Open Cluster Study. LXVI. Spectroscopic Binary Orbits in the Young Open Cluster M35 (NGC 2168) . Leiner, E. M., Mathieu, R. D., et all. . AJ . 150-10 . 2015 . 2015AJ....150...10L ,
The Interacti...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-05-05T15:42:04Z/2008-10-15T07:39:53Z
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 2009-11-15T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-11-15T00:00:00Z, 055351, 17.56_20190403_1200. https://doi.org/10.5270/esa-rercq3l