A dataset provided by the European Space Agency

Name 008636
Title The evolution of stellar coronae from the PMS through the ZAMS
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0086360301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0086360401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0086360901

DOI 10.5270/esa-2y33men
Author Prof Frederick Walter
Description We propose to obtain high quality coronal spectra of 3 pre-main sequence stars, using the RGS, to determine their emission measure distributions and coronal abundances. Together with 3 GTO targets, these stars form a matched grid of cTT, nTT, and ZAMS stars to let us study the evolution of coronal properties from accreting PMS stars through the development of a radiative core, extending studies of the evolution of coronal properties back to ages of 1-2 million years.
Publication A large X-ray flare from the Herbig Ae star V892 Tau . Giardino, G., Favata, F., et all. . A&A . 413-669 . 2004 . 2004A&A...413..669G ,
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 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 ,
The XMM-Newton Optical Monitor survey of the Taurus molecular cloud . Audard, M., Briggs, K. R., et all. . A&A . 468-379 . 2007 . 2007A&A...468..379A ,
X-ray emission from the young brown dwarfs of the Taurus molecular cloud . Grosso, N., Briggs, K. R., et all. . A&A . 468-391 . 2007 . 2007A&A...468..391G ,
New pre-main sequence candidates in the Taurus-Auriga star forming region . Scelsi, L., Maggio, A., et all. . A&A . 468-405 . 2007 . 2007A&A...468..405S ,
The X-ray activity-rotatio...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-03-11T09:40:56Z/2001-03-12T21:51:41Z
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 2002-09-24T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-09-24T00:00:00Z, 008636, 17.56_20190403_1200. https://doi.org/10.5270/esa-2y33men