A dataset provided by the European Space Agency

Name: Probing the X-ray emission from the low mass CTTS DN Tau
Published: 2011-09-21T00:00:00Z

Proposal ID	065112
Title	Probing the X-ray emission from the low mass CTTS DN Tau
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651120101
DOI	https://doi.org/10.5270/esa-fzue7i3
Principal Investigator, PI	Dr Jan Robrade
Abstract	High resolution X-ray spectroscopy of young stellar objects clearly indicatesthat in classical TvirgulTauri stars the physical properties of the cooler X-rayemitting plasma are strongly influenced by accretion and outflow processes. Thedetailed characteristics apparently depend on stellar parameters like mass andradius; however, especially low mass stars are missing in the the existing X-raydata of young, accreting stars. The proposed observation of DN Tau will extendthe current sample into the mass regime of M dwarf precursors and intends toderive a more comprehensive picture of the pre-main sequence evolution of lowmass stars.
Publications	DN Tauri - coronal activity and accretion in a young low-mass CTTS \|Robrade, J., Gudel, M., et al. \| A&A \| 561-124 \| 2014 \| 2014A&A...561A.124R \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Consistent dust and gas models for protoplanetary disks. IV. A panchromatic view of protoplanetary disks \|Dionatos, O., Woitke, P., et al. \| A&A \| 625-66 \| 2019 \| 2019A&A...625A..66D \| http://ui.adsabs.harvard.edu/#abs/2019A&A...625A..66D Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2010-08-18T02:51:23Z/2010-08-19T12:52:04Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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
Keywords	"low mass stars", "outflow processes", "mass regime", "dn tau", "dwarf precursors", "resolution xray spectroscopy", "stellar parameters", "accreting stars", "physical properties", "tauri stars", "xray emission", "comprehensive picture", "stellar objects", "existing xray data", "characteristics apparently depend"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jan Robrade, 2011, 'Probing the X-ray emission from the low mass CTTS DN Tau', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-fzue7i3