A dataset provided by the European Space Agency

Name 010144
Title Evolution of coronal activity from observations of open clusters and SFRs
URL

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DOI 10.5270/esa-5po393z
Author Prof Roberto Pallavicini
Description GT-Open clusters and young stellar associations offer unique opportunities to study the evolution of angular momentum in late-type stars and the dependemce of coronal activity upon age, rotation and mass. We propose to carry out a spectroscopic survey of several nearby open clusters of different ages and of a few star forming regions (SFRs) with the aim of deriving the evolution of coronal properties for stars of different masses. The selected clusters (IC2602, alpha Persei, Hyades and Praesepe) span the age range from 30 Myr to 700 Myr, while the lelected star forming regions (NGC2024 in Orion and Taurus-Auriga) will allow us to further extend this study to ages as young as 1 to 10 Myr. Other clusters and SFRs will be observed by other XMM GT and GO programmes.
Publication Is Praesepe really different from the coeval Hyades cluster? The XMM-Newton view . Franciosini, E., Randich, S., . A&A . 405-551 . 2003 . 2003A&A...405..551F ,
Properties of serendipitous X-ray flares discovered in XMM-Newton observations . Trenholme, Duncan, Ramsay, Gavin, . MNRAS . 355-1125 . 2004 . 2004MNRAS.355.1125T ,
Coronal properties of G-type stars in different evolutionary phases . Scelsi, L., Maggio, A., et all. . A&A . 432-671 . 2005 . 2005A&A...432..671S ,
XMM-Newton observations of the sigma Orionis cluster. II. Spatial and spectral analysis of the full EPIC field . Franciosini, E., Pallavicini, R., . A&A . 446-501 . 2006 . 2006A&A...446..501F ,
The XMM-Newton extended survey of the Taurus molecular cloud (XEST) . Gudel, M., Briggs, K. R., et all. . A&A . 468-353 . 2007 . 2007A&A...468..353G ,
The first high-resolution X-ray spectrum of a Herbig star: AB Aurigae . Telleschi, A., Gudel, M., et all. . A&A . 468-541 . 2007 . 2007A&A...468..541T ,
The enigmatic X-rays from the Herbig star HD 163296: Jet, accretion, or corona? . Gunther, H. M., Schmitt, J. H. M. M., . A&A . 494-1041 . 2009 . 2009A&A...494.1041G ,
Identifying XMM-Newton observations affected by solar wind charge exchange - Part II . Carter, J. A., Sembay, S., . A&A . 527-115 . 2011 . 2011A&A...527A.115C ,
The X...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-09-02T20:36:31Z/2002-08-13T17:29:27Z
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 2003-09-17T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-09-17T00:00:00Z, 010144, 17.56_20190403_1200. https://doi.org/10.5270/esa-5po393z