A dataset provided by the European Space Agency

Name 065112
Title Probing the X-ray emission from the low mass CTTS DN Tau


DOI 10.5270/esa-fzue7i3
Author Dr Jan Robrade
Description High resolution X-ray spectroscopy of young stellar objects clearly indicates that in classical T~Tauri stars the physical properties of the cooler X-ray emitting plasma are strongly influenced by accretion and outflow processes. The detailed characteristics apparently depend on stellar parameters like mass and radius; however, especially low mass stars are missing in the the existing X-ray data of young, accreting stars. The proposed observation of DN Tau will extend the current sample into the mass regime of M dwarf precursors and intends to derive a more comprehensive picture of the pre-main sequence evolution of low mass stars.
Publication DN Tauri - coronal activity and accretion in a young low-mass CTTS . Robrade, J., Gudel, M., et all. . A&A . 561-124 . 2014 . 2014A&A...561A.124R ,
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 ,
Consistent dust and gas models for protoplanetary disks. IV. A panchromatic view of protoplanetary disks . Dionatos, O., Woitke, P., et all. . A&A . 625-66 . 2019 . 2019A&A...625A..66D ,
Instrument EPN, RGS1, OM, RGS2, EMOS1, EMOS2
Temporal Coverage 2010-08-18T02:51:23Z/2010-08-19T12:52:04Z
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 2011-09-21T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-09-21T00:00:00Z, 065112, 17.56_20190403_1200. https://doi.org/10.5270/esa-fzue7i3