A dataset provided by the European Space Agency

Name 015246
Title Restless Days of the Infant Sun
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0152460301

DOI 10.5270/esa-q2h0vil
Author Dr Manuel Guedel
Description The earliest stages of the Sun.s life were fundamentally important for the formation of planetary seeds, physical and chemical processes in the Solar Nebula, the dissipation of left-over molecular material, and the chemistry of the forming planetary atmospheres. Many of these mechanisms are intrinsically related to high-energy processes on or near the forming star. The principal goal of the present proposal is a study of the pre-main sequence high-energy life - or lives - of our Sun by investigating a sample of stars of approximately one solar mass with known ages in the nearby Chamaeleon I star formation region. The large effective area of the XMM-Newton EPIC cameras allows us for the first time to conduct a spectroscopic X-ray study of the pre-main sequence X-ray Sun in Time.
Publication X-ray detection of the substellar twin 2MASS J11011926-7732383 AB . Stelzer, B., Micela, G., . A&A . 474-129 . 2007 . 2007A&A...474..129S ,
On the origin of [NeII] 12.81 mum emission from pre-main sequence stars: Disks, jets, and accretion . Gudel, M., Lahuis, F., et all. . A&A . 519-113 . 2010 . 2010A&A...519A.113G ,
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 XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
C2D Spitzer-IRS spectra of disks around T Tauri stars. V. Spectral decomposition . Olofsson, J., Augereau, J.-C., et all. . A&A . 520-39 . 2010 . 2010A&A...520A..39O ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The XMM Cluster Survey: X-...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-08-18T05:52:19Z/2003-08-18T14:27:48Z
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 2004-09-28T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-09-28T00:00:00Z, 015246, 17.56_20190403_1200. https://doi.org/10.5270/esa-q2h0vil